毎秒の写真・画像 : 報道写真・ニュース映像の提供購入サービス：KYODO NEWS IMAGELINK(イメージリンク)

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In 1822 the French appointed commission to finding the speed of sound in air.

In 1822 the French appointed commission to finding the speed of sound in air. Two hills near Paris chosen for the experiment at Villejuif and Montlhery. On each hill a gun was discharged. Observers on the other hill, by noting the time of flash and time at which they heard report, calculated the speed to be 1,118.152 feet (340.8m) per second. Gay-Lussac, Humboldt and Bouvard at Montlhery; Arago, Mathieu and Prony were at Villejuif. From Amedee Guillemin ‘The Forces of Nature‘, London, 1873. Engraving、クレジット：Ｗｏｒｌｄ　Ｈｉｓｔｏｒｙ　Ａｒｃｈｉｖｅ／ニューズコム／共同通信イメージズ　※エディトリアル使用のみ。広告、プロモーション、商業目的での利用に関してはお問合せください。

商品コード: 2019073103106

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In 1822 the French appointed commission to finding the speed of sound in air.

In 1822 the French appointed commission to finding the speed of sound in air. Two hills near Paris chosen for the experiment at Villejuif and Montlhery. On each hill a gun was discharged. Observers on the other hill, by noting the time of flash and time at which they heard report, calculated the speed to be 1,118.152 feet (340.8m) per second. Gay-Lussac, Humboldt and Bouvard at Montlhery; Arago, Mathieu and Prony were at Villejuif. From Robert Brown ‘Science for All‘, London, c.1880、クレジット：Ｗｏｒｌｄ　Ｈｉｓｔｏｒｙ　Ａｒｃｈｉｖｅ／ニューズコム／共同通信イメージズ　※エディトリアル使用のみ。広告、プロモーション、商業目的での利用に関してはお問合せください。

商品コード: 2019073103032

1952年11月04日

毎秒６万コマの高速カメラ

完成した毎秒６万コマ撮影の超高速度カメラ。レンズ上部（中央矢印）のベルトの回転で心棒が回り中のドラムが回転する（東大理工学研究所植村恒義助教授製作）（２７年内地２８４９）

商品コード: 2006022700293

1957年10月08日

東大のシンクロ・サイクロトロン完成

（３）真空装置　円筒内に多少でも空気があれば粒子の運行にじゃまなので高真空にするのがこの円筒状の真空装置。排気能力毎秒２万４０００リットルの３２インチ油拡散ポンプで日本一、二の高性能（東大原子核研究所）＝１９５７（昭和３２）年１０月８日出稿　（縮刷版掲載なし　３２年内地番号なし　組写真通信で出稿　ネガ袋に記事あり）

商品コード: 2012072000167

1964年05月31日

General Motors Proving Ground

Detroit, Michigan: May, 1964 A Corvair test car on the “glass road“ at the General Motors Proving Ground. The car has photo headlamps and a camera focused on the mirror under the glass surface. The mirror reflects the tire‘s footprint and is photographed at 2200 frames per second at 60 mph.、クレジット：Ｕｎｄｅｒｗｏｏｄ　Ａｒｃｈｉｖｅｓ／Ｕｎｉｖｅｒｓａｌ　Ｉｍａｇｅｓ　Ｇｒｏｕｐ／共同通信イメージズ

商品コード: 2020011005237

1994年10月24日

ジョスリン・ベルとアントニー・ヒューイッシュ Jocelyn Bell and Antony Hewish

The astronomers Jocelyn Bell and Anthony Hewish seen amongst the wires of the radio telescope in East Anglia, England, with which they discovered in 1967 the first pulsar. Pulsars are very compact neutron stars that are spinning around at very high speed (several times per second). They also emit a beam of radiation which, due the pulsar fast rotation, creates a light-house effect. Bell and Hewish were investigating the variability of some radio sources when they discovered a source in Lacerta, which was called LMG1, producing a set of equally spaced radio pulses. In 1974 Hewish won the Nobel Prize for physics for this work.、クレジット：ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2023080905669

1994年10月27日

毎秒１１０字を印字

セイコーエプソンのプリンター「ＭＪ―４５０」

商品コード: 1994102700062

1995年10月23日

印刷ミスは見逃しません

１万円札の束を毎秒３ページ程度のスピードでめくりながら印刷ミスを検査する高橋美保子さん＝東京都北区の大蔵省印刷局滝野川工場（たかはし・みほこ）

商品コード: 1995102300022

2000年05月13日

そろりと旧鹿児島県庁舎２千７百トンが毎秒１ミリ移動

８本のレールの上をそろりそろり動いているのは、旧鹿児島県庁舎の玄関部分。１９２５（大正１４）年に建てられたネオ・ルネサンス様式を基調とした３階建てで、重さ約２７００トン。秒速１ミリはカタツムリよりゆっくりだ。旧庁舎の大部分は新庁舎移転に伴い解体されたが、玄関部分は再利用・保存が決定、約２カ月かけて、１１６メートル先に移動される＝１２日午後、鹿児島市山下町

商品コード: 2000051300043

02:07.89

2007年06月26日

空撮　７月上旬にも貯水率ゼロ　早明浦ダム、放流量決定

四国の水がめ、早明浦ダム（高知県）の貯水率が早ければ７月上旬にもゼロとなる見通しとなり、四国地方整備局と四国四県などでつくる吉野川水系水利用連絡協議会は２６日、電源開発が権利を持つ発電用水（約８１２万トン）の使い方を話し合った。この日の会議では、貯水率がゼロになった場合、香川県向けに毎秒１．７トン、徳島県向けに同１．８トンをそれぞれ緊急放流することが決まった＜映像内容＞早明浦ダム、空撮、撮影日：２００７（平成１９）年６月２６日、撮影場所：高知県

商品コード: 2020020703205

00:15.20

2012年04月23日

Northern white-faced owl

High-speed footage of a northern white-faced owl (Otus leucotis) taking off from a hole in a stone wall. This owl inhabits equatorial Africa north of the equator. Filmed at 500 frames per second (slowed down twenty times).、クレジット：ＧＥＲＡＲＤ　ＬＡＣＺ　ＩＭＡＧＥＳ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022060807241

00:45.36

2012年05月10日

Long-eared owl in flight

High-speed footage of a long-eared owl (Asio otus) in flight, taking off from a tree. Filmed in Normandy, France. Filmed at 500 frames per second (slowed down 20 times).、クレジット：ＧＥＲＡＲＤ　ＬＡＣＺ　ＩＭＡＧＥＳ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022060807188

00:27.00

2012年05月10日

Long-eared owl in flight

High-speed footage of a long-eared owl (Asio otus) in flight, taking off from a tree. Filmed in Normandy, France. Filmed at 500 frames per second (slowed down 20 times).、クレジット：ＧＥＲＡＲＤ　ＬＡＣＺ　ＩＭＡＧＥＳ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022060807183

00:24.64

2012年05月10日

Barn owl in flight

High-speed footage of a barn owl (Tyto alba) in flight, taking off from a tree branch. Filmed in Normandy, France. Filmed at 500 frames per second (slowed down 20 times).、クレジット：ＧＥＲＡＲＤ　ＬＡＣＺ　ＩＭＡＧＥＳ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022060807233

00:21.76

2012年05月10日

Long-eared owl in flight

High-speed footage of a long-eared owl (Asio otus) in flight, taking off from a tree. Filmed in Normandy, France. Filmed at 500 frames per second (slowed down 20 times).、クレジット：ＧＥＲＡＲＤ　ＬＡＣＺ　ＩＭＡＧＥＳ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022060807256

00:15.56

2012年05月10日

Barn owl in flight

High-speed footage of a barn owl (Tyto alba) in flight, taking off from a tree trunk. Filmed in Normandy, France. Filmed at 500 frames per second (slowed down 20 times).、クレジット：ＧＥＲＡＲＤ　ＬＡＣＺ　ＩＭＡＧＥＳ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022060807244

00:48.76

2014年01月09日

Northern lights, timelapse

Timelapse footage of the Aurora Borealis, or northern lights. Auroral displays are caused by interactions between energetic charged particles from the Sun, and the Earth‘s atmosphere. Moving at 400-500 kilometres a second, the charged particles of the solar wind are drawn by Earth‘s magnetic field to the poles, where they collide with gas atoms and molecules, causing them to emit light. Green light is from oxygen atoms, purple light from nitrogen atoms. Filmed in Minnesota, USA, in summer.、クレジット：Ｂｏｂ　Ｃｏｎｚｅｍｉｕｓ／ＷｅａｔｈｅｒＶｉｄｅｏＨＤ．ＴＶ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022061405848

00:33.43

2014年01月09日

Northern lights, timelapse

Timelapse footage of the Aurora Borealis, or northern lights, over a lake. Auroral displays are caused by interactions between energetic charged particles from the Sun, and the Earth‘s atmosphere. Moving at 400-500 kilometres a second, the charged particles of the solar wind are drawn by Earth‘s magnetic field to the poles, where they collide with gas atoms and molecules, causing them to emit light. Green light is from oxygen atoms, purple light from nitrogen atoms. Filmed in Minnesota, USA, on 23rd April 2012.、クレジット：Ｂｏｂ　Ｃｏｎｚｅｍｉｕｓ／ＷｅａｔｈｅｒＶｉｄｅｏＨＤ．ＴＶ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022061405854

00:31.26

2014年01月09日

Northern lights, timelapse

Timelapse footage of the Sun setting followed by Aurora Borealis, or northern lights. Stratocumulus clouds partially obscure the view of the aurora. Auroral displays are caused by interactions between energetic charged particles from the Sun, and the Earth‘s atmosphere. Moving at 400-500 kilometres a second, the charged particles of the solar wind are drawn by Earth‘s magnetic field to the poles, where they collide with gas atoms and molecules, causing them to emit light. Green light is from oxygen atoms, purple light from nitrogen atoms. Filmed in Minnesota, USA, in summer.、クレジット：Ｂｏｂ　Ｃｏｎｚｅｍｉｕｓ／ＷｅａｔｈｅｒＶｉｄｅｏＨＤ．ＴＶ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022061405855

00:21.83

2014年01月09日

Northern lights, timelapse

Timelapse footage of the Aurora Borealis, or northern lights, using a fish-eye lens. Auroral displays are caused by interactions between energetic charged particles from the Sun, and the Earth‘s atmosphere. Moving at 400-500 kilometres a second, the charged particles of the solar wind are drawn by Earth‘s magnetic field to the poles, where they collide with gas atoms and molecules, causing them to emit light. Green light is from oxygen atoms, purple light from nitrogen atoms. Filmed in Minnesota, USA.、クレジット：Ｂｏｂ　Ｃｏｎｚｅｍｉｕｓ／ＷｅａｔｈｅｒＶｉｄｅｏＨＤ．ＴＶ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022061405859

00:23.83

2014年01月09日

Northern lights, timelapse

Timelapse footage of the Aurora Borealis, or northern lights, above a layer of stratocumulus clouds. Beneath the clouds is the glow from city lights. Auroral displays are caused by interactions between energetic charged particles from the Sun, and the Earth‘s atmosphere. Moving at 400-500 kilometres a second, the charged particles of the solar wind are drawn by Earth‘s magnetic field to the poles, where they collide with gas atoms and molecules, causing them to emit light. Green light is from oxygen atoms. Filmed in Minnesota, USA, in spring.、クレジット：Ｂｏｂ　Ｃｏｎｚｅｍｉｕｓ／ＷｅａｔｈｅｒＶｉｄｅｏＨＤ．ＴＶ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022061405892

00:19.86

2014年01月09日

Northern lights, timelapse

Timelapse footage of the Aurora Borealis, or northern lights, using a fish-eye lens. Auroral displays are caused by interactions between energetic charged particles from the Sun, and the Earth‘s atmosphere. Moving at 400-500 kilometres a second, the charged particles of the solar wind are drawn by Earth‘s magnetic field to the poles, where they collide with gas atoms and molecules, causing them to emit light. Green light is from oxygen atoms, purple light from nitrogen atoms. Filmed in Minnesota, USA, on 5th September.、クレジット：Ｂｏｂ　Ｃｏｎｚｅｍｉｕｓ／ＷｅａｔｈｅｒＶｉｄｅｏＨＤ．ＴＶ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022061405850

00:13.20

2014年01月09日

Northern lights, timelapse

Timelapse footage of the Aurora Borealis, or northern lights, over a lake. The aurorae are partially obscured by altocumulus clouds. Auroral displays are caused by interactions between energetic charged particles from the Sun, and the Earth‘s atmosphere. Moving at 400-500 kilometres a second, the charged particles of the solar wind are drawn by Earth‘s magnetic field to the poles, where they collide with gas atoms and molecules, causing them to emit light. Green light is from oxygen atoms, purple light from nitrogen atoms. Filmed in Minnesota, USA, in spring.、クレジット：Ｂｏｂ　Ｃｏｎｚｅｍｉｕｓ／ＷｅａｔｈｅｒＶｉｄｅｏＨＤ．ＴＶ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022061405887

00:15.70

2014年01月09日

Northern lights, timelapse

Timelapse footage of the Aurora Borealis, or northern lights, over a lake. Auroral displays are caused by interactions between energetic charged particles from the Sun, and the Earth‘s atmosphere. Moving at 400-500 kilometres a second, the charged particles of the solar wind are drawn by Earth‘s magnetic field to the poles, where they collide with gas atoms and molecules, causing them to emit light. Green light is from oxygen atoms, purple light from nitrogen atoms. Filmed in Minnesota, USA, in spring.、クレジット：Ｂｏｂ　Ｃｏｎｚｅｍｉｕｓ／ＷｅａｔｈｅｒＶｉｄｅｏＨＤ．ＴＶ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022061405897

00:05.83

2014年01月09日

Northern lights, timelapse

Timelapse footage of the Aurora Borealis, or northern lights. Auroral displays are caused by interactions between energetic charged particles from the Sun, and the Earth‘s atmosphere. Moving at 400-500 kilometres a second, the charged particles of the solar wind are drawn by Earth‘s magnetic field to the poles, where they collide with gas atoms and molecules, causing them to emit light. Green light is from oxygen atoms, purple light from nitrogen atoms. Filmed in Minnesota, USA.、クレジット：Ｂｏｂ　Ｃｏｎｚｅｍｉｕｓ／ＷｅａｔｈｅｒＶｉｄｅｏＨＤ．ＴＶ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022061405899

00:23.46

2014年01月09日

Northern lights, timelapse

Timelapse footage of the Aurora Borealis, or northern lights. They are eventually blocked by dense cirrus clouds. Auroral displays are caused by interactions between energetic charged particles from the Sun, and the Earth‘s atmosphere. Moving at 400-500 kilometres a second, the charged particles of the solar wind are drawn by Earth‘s magnetic field to the poles, where they collide with gas atoms and molecules, causing them to emit light. Green light is from oxygen atoms, purple light from nitrogen atoms. Filmed in Minnesota, USA.、クレジット：Ｂｏｂ　Ｃｏｎｚｅｍｉｕｓ／ＷｅａｔｈｅｒＶｉｄｅｏＨＤ．ＴＶ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022061405840

00:22.26

2014年01月09日

Northern lights, timelapse

Timelapse footage of the Aurora Borealis, or northern lights. Auroral displays are caused by interactions between energetic charged particles from the Sun, and the Earth‘s atmosphere. Moving at 400-500 kilometres a second, the charged particles of the solar wind are drawn by Earth‘s magnetic field to the poles, where they collide with gas atoms and molecules, causing them to emit light. Purple light is from nitrogen atoms. Filmed in Minnesota, USA, in November 2012.、クレジット：Ｂｏｂ　Ｃｏｎｚｅｍｉｕｓ／ＷｅａｔｈｅｒＶｉｄｅｏＨＤ．ＴＶ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022061405846

00:20.13

2014年01月09日

Northern lights, timelapse

Timelapse footage of the Aurora Borealis, or northern lights. Auroral displays are caused by interactions between energetic charged particles from the Sun, and the Earth‘s atmosphere. Moving at 400-500 kilometres a second, the charged particles of the solar wind are drawn by Earth‘s magnetic field to the poles, where they collide with gas atoms and molecules, causing them to emit light. Green light is from oxygen atoms, purple light from nitrogen atoms. Filmed in Minnesota, USA, in summer.、クレジット：Ｂｏｂ　Ｃｏｎｚｅｍｉｕｓ／ＷｅａｔｈｅｒＶｉｄｅｏＨＤ．ＴＶ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022061405864

00:16.93

2014年01月09日

Northern lights, timelapse

Timelapse footage of the Aurora Borealis, or northern lights, partly seen through thin cirrus clouds. Auroral displays are caused by interactions between energetic charged particles from the Sun, and the Earth‘s atmosphere. Moving at 400-500 kilometres a second, the charged particles of the solar wind are drawn by Earth‘s magnetic field to the poles, where they collide with gas atoms and molecules, causing them to emit light. Green light is from oxygen atoms, purple light from nitrogen atoms. Filmed in Minnesota, USA, on 13th April 2012.、クレジット：Ｂｏｂ　Ｃｏｎｚｅｍｉｕｓ／ＷｅａｔｈｅｒＶｉｄｅｏＨＤ．ＴＶ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022061405889

00:15.50

2014年01月09日

Northern lights, timelapse

Timelapse footage of the Aurora Borealis, or northern lights, in a moon-lit sky. Auroral displays are caused by interactions between energetic charged particles from the Sun, and the Earth‘s atmosphere. Moving at 400-500 kilometres a second, the charged particles of the solar wind are drawn by Earth‘s magnetic field to the poles, where they collide with gas atoms and molecules, causing them to emit light. Green light is from oxygen atoms, purple light from nitrogen atoms. Filmed in Minnesota, USA, in winter.、クレジット：Ｂｏｂ　Ｃｏｎｚｅｍｉｕｓ／ＷｅａｔｈｅｒＶｉｄｅｏＨＤ．ＴＶ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022061405880

00:11.20

2014年01月09日

Northern lights, timelapse

Timelapse footage of the Aurora Borealis, or northern lights. Auroral displays are caused by interactions between energetic charged particles from the Sun, and the Earth‘s atmosphere. Moving at 400-500 kilometres a second, the charged particles of the solar wind are drawn by Earth‘s magnetic field to the poles, where they collide with gas atoms and molecules, causing them to emit light. Green light is from oxygen atoms, purple light from nitrogen atoms. Filmed in Minnesota, USA, in summer.、クレジット：Ｂｏｂ　Ｃｏｎｚｅｍｉｕｓ／ＷｅａｔｈｅｒＶｉｄｅｏＨＤ．ＴＶ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022061405890

00:16.53

2014年01月09日

Northern lights, timelapse

Timelapse footage of the Aurora Borealis, or northern lights, over water. Auroral displays are caused by interactions between energetic charged particles from the Sun, and the Earth‘s atmosphere. Moving at 400-500 kilometres a second, the charged particles of the solar wind are drawn by Earth‘s magnetic field to the poles, where they collide with gas atoms and molecules, causing them to emit light. Green light is from oxygen atoms, purple light from nitrogen atoms. Filmed in Minnesota, USA, in spring.、クレジット：Ｂｏｂ　Ｃｏｎｚｅｍｉｕｓ／ＷｅａｔｈｅｒＶｉｄｅｏＨＤ．ＴＶ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022061405857

00:30.96

2014年01月09日

Northern lights, timelapse

Timelapse footage of the Aurora Borealis, or northern lights, in a moon-lit sky. Auroral displays are caused by interactions between energetic charged particles from the Sun, and the Earth‘s atmosphere. Moving at 400-500 kilometres a second, the charged particles of the solar wind are drawn by Earth‘s magnetic field to the poles, where they collide with gas atoms and molecules, causing them to emit light. Green light is from oxygen atoms, purple light from nitrogen atoms. Filmed in Minnesota, USA, in winter.、クレジット：Ｂｏｂ　Ｃｏｎｚｅｍｉｕｓ／ＷｅａｔｈｅｒＶｉｄｅｏＨＤ．ＴＶ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022061405877

00:28.06

2014年01月09日

Northern lights, timelapse

Timelapse footage of the Aurora Borealis, or northern lights. Auroral displays are caused by interactions between energetic charged particles from the Sun, and the Earth‘s atmosphere. Moving at 400-500 kilometres a second, the charged particles of the solar wind are drawn by Earth‘s magnetic field to the poles, where they collide with gas atoms and molecules, causing them to emit light. Green light is from oxygen atoms, purple light from nitrogen atoms. It is very uncommon for aurorae to be nearly overhead at mid-latitudes. Filmed in Minnesota, USA, in summer.、クレジット：Ｂｏｂ　Ｃｏｎｚｅｍｉｕｓ／ＷｅａｔｈｅｒＶｉｄｅｏＨＤ．ＴＶ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022061405898

00:17.66

2014年01月09日

Northern lights, timelapse

Timelapse footage of the Aurora Borealis, or northern lights. Auroral displays are caused by interactions between energetic charged particles from the Sun, and the Earth‘s atmosphere. Moving at 400-500 kilometres a second, the charged particles of the solar wind are drawn by Earth‘s magnetic field to the poles, where they collide with gas atoms and molecules, causing them to emit light. Green light is from oxygen atoms, purple light from nitrogen atoms. Filmed in northern Minnesota, USA.、クレジット：Ｂｏｂ　Ｃｏｎｚｅｍｉｕｓ／ＷｅａｔｈｅｒＶｉｄｅｏＨＤ．ＴＶ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022061405868

01:19.96

2014年01月09日

Northern lights, timelapse

Timelapse footage of the Aurora Borealis, or northern lights. Auroral displays are caused by interactions between energetic charged particles from the Sun, and the Earth‘s atmosphere. Moving at 400-500 kilometres a second, the charged particles of the solar wind are drawn by Earth‘s magnetic field to the poles, where they collide with gas atoms and molecules, causing them to emit light. Green light is from oxygen atoms, purple light from nitrogen atoms. Filmed in Minnesota, USA, in May 2012.、クレジット：Ｂｏｂ　Ｃｏｎｚｅｍｉｕｓ／ＷｅａｔｈｅｒＶｉｄｅｏＨＤ．ＴＶ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022061405881

00:27.26

2014年01月09日

Northern lights, timelapse

Timelapse footage of the Aurora Borealis, or northern lights, in a moon-lit sky. Auroral displays are caused by interactions between energetic charged particles from the Sun, and the Earth‘s atmosphere. Moving at 400-500 kilometres a second, the charged particles of the solar wind are drawn by Earth‘s magnetic field to the poles, where they collide with gas atoms and molecules, causing them to emit light. Green light is from oxygen atoms, purple light from nitrogen atoms. Filmed in Minnesota, USA, in winter.、クレジット：Ｂｏｂ　Ｃｏｎｚｅｍｉｕｓ／ＷｅａｔｈｅｒＶｉｄｅｏＨＤ．ＴＶ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022061405871

00:33.10

2014年01月09日

Northern lights, timelapse

Timelapse footage of the Aurora Borealis, or northern lights, over a lake. Auroral displays are caused by interactions between energetic charged particles from the Sun, and the Earth‘s atmosphere. Moving at 400-500 kilometres a second, the charged particles of the solar wind are drawn by Earth‘s magnetic field to the poles, where they collide with gas atoms and molecules, causing them to emit light. Green light is from oxygen atoms, purple light from nitrogen atoms. Filmed in Minnesota, USA.、クレジット：Ｂｏｂ　Ｃｏｎｚｅｍｉｕｓ／ＷｅａｔｈｅｒＶｉｄｅｏＨＤ．ＴＶ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022061405843

00:10.00

2014年01月09日

Northern lights, timelapse

Timelapse footage of the Aurora Borealis, or northern lights, in a moon-lit sky. Auroral displays are caused by interactions between energetic charged particles from the Sun, and the Earth‘s atmosphere. Moving at 400-500 kilometres a second, the charged particles of the solar wind are drawn by Earth‘s magnetic field to the poles, where they collide with gas atoms and molecules, causing them to emit light. Green light is from oxygen atoms, purple light from nitrogen atoms. Filmed in Minnesota, USA, in winter.、クレジット：Ｂｏｂ　Ｃｏｎｚｅｍｉｕｓ／ＷｅａｔｈｅｒＶｉｄｅｏＨＤ．ＴＶ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022061405893

00:17.33

2014年01月09日

Northern lights, timelapse

Timelapse footage of the Aurora Borealis, or northern lights, in a moon-lit sky. Auroral displays are caused by interactions between energetic charged particles from the Sun, and the Earth‘s atmosphere. Moving at 400-500 kilometres a second, the charged particles of the solar wind are drawn by Earth‘s magnetic field to the poles, where they collide with gas atoms and molecules, causing them to emit light. Green light is from oxygen atoms, purple light from nitrogen atoms. Filmed in Minnesota, USA, in winter.、クレジット：Ｂｏｂ　Ｃｏｎｚｅｍｉｕｓ／ＷｅａｔｈｅｒＶｉｄｅｏＨＤ．ＴＶ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022061405845

00:12.66

2014年01月09日

Northern lights, timelapse

Timelapse footage of the Aurora Borealis, or northern lights, over a lake. Auroral displays are caused by interactions between energetic charged particles from the Sun, and the Earth‘s atmosphere. Moving at 400-500 kilometres a second, the charged particles of the solar wind are drawn by Earth‘s magnetic field to the poles, where they collide with gas atoms and molecules, causing them to emit light. Green light is from oxygen atoms, purple light from nitrogen atoms. Filmed in Minnesota, USA, in spring.、クレジット：Ｂｏｂ　Ｃｏｎｚｅｍｉｕｓ／ＷｅａｔｈｅｒＶｉｄｅｏＨＤ．ＴＶ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022061405853

00:20.53

2014年01月09日

Northern lights, timelapse

Timelapse footage of the Aurora Borealis, or northern lights, over a lake. Auroral displays are caused by interactions between energetic charged particles from the Sun, and the Earth‘s atmosphere. Moving at 400-500 kilometres a second, the charged particles of the solar wind are drawn by Earth‘s magnetic field to the poles, where they collide with gas atoms and molecules, causing them to emit light. Green light is from oxygen atoms, purple light from nitrogen atoms. Filmed in Minnesota, USA.、クレジット：Ｂｏｂ　Ｃｏｎｚｅｍｉｕｓ／ＷｅａｔｈｅｒＶｉｄｅｏＨＤ．ＴＶ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022061405867

01:06.60

2014年01月09日

Northern lights, timelapse

Timelapse footage of the Sun setting followed by Aurora Borealis, or northern lights. A fish-eye lens view is then seen, until the Sun rises. Auroral displays are caused by interactions between energetic charged particles from the Sun, and the Earth‘s atmosphere. Moving at 400-500 kilometres a second, the charged particles of the solar wind are drawn by Earth‘s magnetic field to the poles, where they collide with gas atoms and molecules, causing them to emit light. Green light is from oxygen atoms, purple light from nitrogen atoms. Filmed in Minnesota, USA, in spring.、クレジット：Ｂｏｂ　Ｃｏｎｚｅｍｉｕｓ／ＷｅａｔｈｅｒＶｉｄｅｏＨＤ．ＴＶ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022061405872

00:19.46

2014年01月09日

Northern lights, timelapse

Timelapse footage of the Aurora Borealis, or northern lights. Auroral displays are caused by interactions between energetic charged particles from the Sun, and the Earth‘s atmosphere. Moving at 400-500 kilometres a second, the charged particles of the solar wind are drawn by Earth‘s magnetic field to the poles, where they collide with gas atoms and molecules, causing them to emit light. Green light is from oxygen atoms. Filmed in Minnesota, USA.、クレジット：Ｓｋｙ　Ｆｉｒｅ／ＷｅａｔｈｅｒＶｉｄｅｏＨＤ．ＴＶ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022061405882

00:16.78

2014年01月13日

Northern lights, timelapse

Timelapse footage of the Aurora Borealis, or northern lights, spanning the horizon. Auroral displays are caused by interactions between energetic charged particles from the Sun, and the Earth‘s atmosphere. Moving at 400-500 kilometres a second, the charged particles of the solar wind are drawn by Earth‘s magnetic field to the poles, where they collide with gas atoms and molecules, causing them to emit light. Green light is from oxygen atoms, purple light from nitrogen atoms. Filmed in the USA.、クレジット：Ｔｏｍ　Ｗａｒｎｅｒ／ＷｅａｔｈｅｒＶｉｄｅｏＨＤ．ＴＶ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022061405858

02:35.65

2015年06月15日

満濃池で「ゆる抜き」　讃岐地方、初夏の風物詩

讃岐地方の初夏の風物詩で、水田用に水門を開放する「ゆる抜き」が１５日、国内最大級のかんがい用ため池、香川県まんのう町の満濃池で行われた。池の水門から毎秒５トンの水が勢いよく流れ出すと、集まった大勢の観光客から歓声が上がった。今後、下流地域の田植えが本格化する。〈映像内容〉満濃池からしぶきを上げて水が流れ出す様子、撮影日：２０１５（平成２７）年６月１５日、撮影場所：讃岐地方

商品コード: 2019031300837

2015年09月19日

関電の黒部ルート電力需要支えた歴史知る

壁面の高さが１８６㍍と日本一を誇る黒部ダム。１０月１５日までの日中、毎秒１０～１５㌧の水が放流される＝８月、富山県立山町

商品コード: 2015091900064

2016年04月12日

French Government Will Support Struggling Atos To Save Jobs

File photo - Atmosphere during the presentation of Atos‘ Bull Sequana, the world‘s most efficient supercomputer, at Loft Sevigne showroom in Paris, France on April 12, 2016. A first exascale-class computer, Bull Sequana is capable of processing a billion billion operations per second while consuming 10 times less energy than current systems. - The French government will be there to support the activities of Atos and the tens of thousands of jobs employed by the struggling IT services group, French Finance Minister Bruno Le Maire, after Atos shares plunged around 29 %. On Monday, Atos said it would drop plans for a rights issue due to “changes in the market environment“ and added it had started talks with its banks about refinancing its debt. Photo by Christian Liewig/ABACAPRESS.COM、クレジット：Ｌｉｅｗｉｇ　Ｃｈｒｉｓｔｉａｎ／ＡＢＡＣＡ／共同通信イメージズ

商品コード: 2024020610222

2016年04月12日

French Government Will Support Struggling Atos To Save Jobs

File photo - Atos Chairman and CEO Thierry Breton delivers his speech during the presentation of Atos‘ Bull Sequana, the world‘s most efficient supercomputer, at Loft Sevigne showroom in Paris, France on April 12, 2016. A first exascale-class computer, Bull Sequana is capable of processing a billion billion operations per second while consuming 10 times less energy than current systems. - The French government will be there to support the activities of Atos and the tens of thousands of jobs employed by the struggling IT services group, French Finance Minister Bruno Le Maire, after Atos shares plunged around 29 %. On Monday, Atos said it would drop plans for a rights issue due to “changes in the market environment“ and added it had started talks with its banks about refinancing its debt. Photo by Christian Liewig/ABACAPRESS.COM、クレジット：Ｌｉｅｗｉｇ　Ｃｈｒｉｓｔｉａｎ／ＡＢＡＣＡ／共同通信イメージズ

商品コード: 2024020610221

2016年04月12日

French Government Will Support Struggling Atos To Save Jobs

File photo - Atos Chairman and CEO Thierry Breton delivers his speech during the presentation of Atos‘ Bull Sequana, the world‘s most efficient supercomputer, at Loft Sevigne showroom in Paris, France on April 12, 2016. A first exascale-class computer, Bull Sequana is capable of processing a billion billion operations per second while consuming 10 times less energy than current systems. - The French government will be there to support the activities of Atos and the tens of thousands of jobs employed by the struggling IT services group, French Finance Minister Bruno Le Maire, after Atos shares plunged around 29 %. On Monday, Atos said it would drop plans for a rights issue due to “changes in the market environment“ and added it had started talks with its banks about refinancing its debt. Photo by Christian Liewig/ABACAPRESS.COM、クレジット：Ｌｉｅｗｉｇ　Ｃｈｒｉｓｔｉａｎ／ＡＢＡＣＡ／共同通信イメージズ

商品コード: 2024020610232

2016年04月12日

French Government Will Support Struggling Atos To Save Jobs

File photo - French Minister of the Economy, Industry and the Digital Sector Emmanuel Macron and Atos Chairman and CEO Thierry Breton at Loft Sevigne showroom for the presentation of Atos‘ Bull Sequana, the world‘s most efficient supercomputer, in Paris, France on April 12, 2016. A first exascale-class computer, Bull Sequana is capable of processing a billion billion operations per second while consuming 10 times less energy than current systems. - The French government will be there to support the activities of Atos and the tens of thousands of jobs employed by the struggling IT services group, French Finance Minister Bruno Le Maire, after Atos shares plunged around 29 %. On Monday, Atos said it would drop plans for a rights issue due to “changes in the market environment“ and added it had started talks with its banks about refinancing its debt. Photo by Christian Liewig/ABACAPRESS.COM、クレジット：Ｌｉｅｗｉｇ　Ｃｈｒｉｓｔｉａｎ／ＡＢＡＣＡ／共同通信イメージズ

商品コード: 2024020610225

2016年04月12日

French Government Will Support Struggling Atos To Save Jobs

File photo - French Minister of the Economy, Industry and the Digital Sector Emmanuel Macron and Atos Chairman and CEO Thierry Breton at Loft Sevigne showroom for the presentation of Atos‘ Bull Sequana, the world‘s most efficient supercomputer, in Paris, France on April 12, 2016. A first exascale-class computer, Bull Sequana is capable of processing a billion billion operations per second while consuming 10 times less energy than current systems. - The French government will be there to support the activities of Atos and the tens of thousands of jobs employed by the struggling IT services group, French Finance Minister Bruno Le Maire, after Atos shares plunged around 29 %. On Monday, Atos said it would drop plans for a rights issue due to “changes in the market environment“ and added it had started talks with its banks about refinancing its debt. Photo by Christian Liewig/ABACAPRESS.COM、クレジット：Ｌｉｅｗｉｇ　Ｃｈｒｉｓｔｉａｎ／ＡＢＡＣＡ／共同通信イメージズ

商品コード: 2024020610162

2016年04月12日

French Government Will Support Struggling Atos To Save Jobs

File photo - French Minister of the Economy, Industry and the Digital Sector Emmanuel Macron and Atos Chairman and CEO Thierry Breton at Loft Sevigne showroom for the presentation of Atos‘ Bull Sequana, the world‘s most efficient supercomputer, in Paris, France on April 12, 2016. A first exascale-class computer, Bull Sequana is capable of processing a billion billion operations per second while consuming 10 times less energy than current systems. - The French government will be there to support the activities of Atos and the tens of thousands of jobs employed by the struggling IT services group, French Finance Minister Bruno Le Maire, after Atos shares plunged around 29 %. On Monday, Atos said it would drop plans for a rights issue due to “changes in the market environment“ and added it had started talks with its banks about refinancing its debt. Photo by Christian Liewig/ABACAPRESS.COM、クレジット：Ｌｉｅｗｉｇ　Ｃｈｒｉｓｔｉａｎ／ＡＢＡＣＡ／共同通信イメージズ

商品コード: 2024020610230

2016年04月12日

French Government Will Support Struggling Atos To Save Jobs

File photo - French Minister of the Economy, Industry and the Digital Sector Emmanuel Macron and Atos Chairman and CEO Thierry Breton at Loft Sevigne showroom for the presentation of Atos‘ Bull Sequana, the world‘s most efficient supercomputer, in Paris, France on April 12, 2016. A first exascale-class computer, Bull Sequana is capable of processing a billion billion operations per second while consuming 10 times less energy than current systems. - The French government will be there to support the activities of Atos and the tens of thousands of jobs employed by the struggling IT services group, French Finance Minister Bruno Le Maire, after Atos shares plunged around 29 %. On Monday, Atos said it would drop plans for a rights issue due to “changes in the market environment“ and added it had started talks with its banks about refinancing its debt. Photo by Christian Liewig/ABACAPRESS.COM、クレジット：Ｌｉｅｗｉｇ　Ｃｈｒｉｓｔｉａｎ／ＡＢＡＣＡ／共同通信イメージズ

商品コード: 2024020610227

2016年04月12日

French Government Will Support Struggling Atos To Save Jobs

File photo - French Minister of the Economy, Industry and the Digital Sector Emmanuel Macron during the presentation of Atos‘ Bull Sequana, the world‘s most efficient supercomputer, at Loft Sevigne showroom in Paris, France on April 12, 2016. A first exascale-class computer, Bull Sequana is capable of processing a billion billion operations per second while consuming 10 times less energy than current systems. - The French government will be there to support the activities of Atos and the tens of thousands of jobs employed by the struggling IT services group, French Finance Minister Bruno Le Maire, after Atos shares plunged around 29 %. On Monday, Atos said it would drop plans for a rights issue due to “changes in the market environment“ and added it had started talks with its banks about refinancing its debt. Photo by Christian Liewig/ABACAPRESS.COM、クレジット：Ｌｉｅｗｉｇ　Ｃｈｒｉｓｔｉａｎ／ＡＢＡＣＡ／共同通信イメージズ

商品コード: 2024020610168

2016年04月12日

French Government Will Support Struggling Atos To Save Jobs

File photo - French Minister of the Economy, Industry and the Digital Sector Emmanuel Macron and Atos Chairman and CEO Thierry Breton at Loft Sevigne showroom for the presentation of Atos‘ Bull Sequana, the world‘s most efficient supercomputer, in Paris, France on April 12, 2016. A first exascale-class computer, Bull Sequana is capable of processing a billion billion operations per second while consuming 10 times less energy than current systems. - The French government will be there to support the activities of Atos and the tens of thousands of jobs employed by the struggling IT services group, French Finance Minister Bruno Le Maire, after Atos shares plunged around 29 %. On Monday, Atos said it would drop plans for a rights issue due to “changes in the market environment“ and added it had started talks with its banks about refinancing its debt. Photo by Christian Liewig/ABACAPRESS.COM、クレジット：Ｌｉｅｗｉｇ　Ｃｈｒｉｓｔｉａｎ／ＡＢＡＣＡ／共同通信イメージズ

商品コード: 2024020610165

01:05.33

2016年08月05日

「東奥日報」ジャガイモ収穫が最盛期／横浜

県内有数のジャガイモ生産地・横浜町で、収穫が最盛期を迎えている。５日、同町大豆田（まめだ）地区にある二木春美さん（６２）の畑では、毎秒２０数個の速度で収穫できる大型機械「ポテトハーベスター」で、大量のジャガイモを一気に掘り取っていた。＜映像内容＞ジャガイモの収穫の様子、撮影日：２０１６（平成２８）年８月５日、撮影場所：青森県横浜町、クレジット：東奥日報／共同通信イメージズ　※白素材

商品コード: 2018020100797

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2018年07月14日

三峡ダム、今年の最高水位迎える

１４日、湖北省宜昌市秭帰県茅坪镇で撮影した排水門から排水を行う三峡ダム。（小型無人機から）中国の長江水利委員会水文局は１３日、今年２回目の洪水が長江上流で発生しており、湖北省宜昌市の三峡ダムはすでに今年の洪水期の最高水位を迎えたと発表した。長江三峡集団のホームページによると、三峡ダムの流入量は１４日午後２時の時点で毎秒５万９６００立方メートルに達し、１５日午前８時には毎秒５万６５００立方メートルまで減少している。（宜昌＝新華社配信／王罡撮影）＝２０１８（平成３０）年７月１４日、クレジット：新華社／共同通信イメージズ

商品コード: 2018071700675

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2018年07月14日

三峡ダム、今年の最高水位迎える

１４日、湖北省宜昌市秭帰県で撮影した三峡ダム。中国の長江水利委員会水文局は１３日、今年２回目の洪水が長江上流で発生しており、湖北省宜昌市の三峡ダムはすでに今年の洪水期の最高水位を迎えたと発表した。長江三峡集団のホームページによると、三峡ダムの流入量は１４日午後２時の時点で毎秒５万９６００立方メートルに達し、１５日午前８時には毎秒５万６５００立方メートルまで減少している。（宜昌＝新華社配信／王罡撮影）＝２０１８（平成３０）年７月１４日、クレジット：新華社／共同通信イメージズ

商品コード: 2018071700609

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01:04.60

2018年12月14日

「新華社」黄河に流氷出現陝西省大茘県

中国陝西省渭南市大茘県はこのところ、低い気温の日々が続き、県内を流れる黄河では４０キロメートル近くにわたり流氷が見られた。川面全体の流氷の密度は高く、川岸や河原にも結氷が確認され、流氷は「千軍万馬」のように流れ寄せ、黄河の壮麗な景観を作り出した。水利部門の観測データによると、同県より上流に位置する山西省河津市にある黄河の竜門での水流は１４日午前８時時点で毎秒約４０６立方メートル、流氷の密度は２０～３０％、氷の厚さは３～５センチだった。気温の低下と上流の流氷の変化による影響を防ぐため、現地の洪水対策部門は既に監視を強化し、流氷の状況の変化を注意深く見守り、増水対策を徹底し、黄河の流氷が何事もなく通過するよう対策を立てている。（記者／都紅剛、李浩）＜映像内容＞黄河の流氷の様子、撮影日：２０１８（平成３０）年１２月１４日、クレジット：新華社／共同通信イメージズ

商品コード: 2018121704850

2019年02月07日

5G technology

07 February 2019, Hamburg: An antenna receiving unit with a 5G modem (Fixed Wireless Access FWA) stands next to a laptop on which a speed test indicates a download rate of 0.00 Gigabit per second (Gbps). Shortly before the completion of a test of high-speed Internet connections based on 5G technology in Hamburg, Telefónica Germany has drawn a positive interim balance. With 5G frequencies in the 26 GHz band used for the first time in this test, it is possible to surf the Internet at lightning speed with several gigabits per second. Photo: Christian Charisius/dpa、クレジット：ＤＰＡ／共同通信イメージズ

商品コード: 2019030300520

2019年02月07日

5G technology

07 February 2019, Hamburg: An antenna receiving unit with 5G modem (Fixed Wireless Access FWA) stands next to a laptop on which a speed test indicates a download rate of 1.01 Gigabit per second (Gbps). Shortly before the completion of a test of high-speed Internet connections based on 5G technology in Hamburg, Telefónica Germany has drawn a positive interim balance. With 5G frequencies in the 26 GHz band used for the first time in this test, it is possible to surf the Internet at lightning speed with several gigabits per second. Photo: Christian Charisius/dpa、クレジット：ＤＰＡ／共同通信イメージズ

商品コード: 2019030300555

2019年02月07日

5G technology

07 February 2019, Hamburg: An antenna receiving unit with 5G modem (Fixed Wireless Access FWA) stands next to a laptop running a speed test. Shortly before the completion of a test of high-speed Internet connections based on 5G technology in Hamburg, Telefónica Germany has drawn a positive interim balance. With 5G frequencies in the 26 GHz band used for the first time in this test, it is possible to surf the Internet at lightning speed with several gigabits per second. Photo: Christian Charisius/dpa、クレジット：ＤＰＡ／共同通信イメージズ

商品コード: 2019030300726

2019年02月07日

Press conference 5G Internet supply

07 February 2019, Hamburg: An antenna receiving unit with 5G modem (Fixed Wireless Access FWA) stands next to a laptop on which a speed test indicates a download rate of 1.02 Gigabit per second (Gbps). Shortly before the completion of a test of high-speed Internet connections based on 5G technology in Hamburg, Telefónica Germany has drawn a positive interim balance. With 5G frequencies in the 26 GHz band used for the first time in this test, it is possible to surf the Internet at lightning speed with several gigabits per second. Photo: Christian Charisius/dpa、クレジット：ＤＰＡ／共同通信イメージズ

商品コード: 2019020827247

2019年02月07日

Press conference 5G Internet supply

07 February 2019, Hamburg: An antenna receiving unit with 5G modem (Fixed Wireless Access FWA) stands next to a laptop on which a speed test indicates a download rate of 0.99 Gigabit per second (Gbps). Shortly before the completion of a test of high-speed Internet connections based on 5G technology in Hamburg, Telefónica Germany has drawn a positive interim balance. With 5G frequencies in the 26 GHz band used for the first time in this test, it is possible to surf the Internet at lightning speed with several gigabits per second. Photo: Christian Charisius/dpa、クレジット：ＤＰＡ／共同通信イメージズ

商品コード: 2019020827248

2019年02月07日

Press conference 5G Internet supply

07 February 2019, Hamburg: A fiber optic fed antenna unit for 5G is mounted on a roof. Shortly before the completion of a test of high-speed Internet connections based on 5G technology in Hamburg, Telefónica Germany has drawn a positive interim balance. With 5G frequencies in the 26 GHz band used for the first time in this test, it is possible to surf the Internet at lightning speed with several gigabits per second. Photo: Christian Charisius/dpa、クレジット：ＤＰＡ／共同通信イメージズ

商品コード: 2019020827427

2019年02月07日

5G technology

07 February 2019, Hamburg: An antenna receiving unit with a 5G modem (Fixed Wireless Access FWA) stands next to a laptop on which a speed test indicates a download rate of 0.00 Gigabit per second (Gbps). Shortly before the completion of a test of high-speed Internet connections based on 5G technology in Hamburg, Telefónica Germany has drawn a positive interim balance. With 5G frequencies in the 26 GHz band used for the first time in this test, it is possible to surf the Internet at lightning speed with several gigabits per second. Photo: Christian Charisius/dpa、クレジット：ＤＰＡ／共同通信イメージズ

商品コード: 2019030300847

2019年02月07日

5G technology

07 February 2019, Hamburg: An antenna reception unit with a 5G modem (Fixed Wireless Access FWA) is on a table during a press conference. Shortly before the completion of a test of high-speed Internet connections based on 5G technology in Hamburg, Telefónica Germany has drawn a positive interim balance. With 5G frequencies in the 26 GHz band used for the first time in this test, it is possible to surf the Internet at lightning speed with several gigabits per second. Photo: Christian Charisius/dpa、クレジット：ＤＰＡ／共同通信イメージズ

商品コード: 2019030300512

2019年02月07日

Press conference 5G Internet supply

07 February 2019, Hamburg: An antenna reception unit with a 5G modem (Fixed Wireless Access FWA) is on a table during a press conference. Shortly before the completion of a test of high-speed Internet connections based on 5G technology in Hamburg, Telefónica Germany has drawn a positive interim balance. With 5G frequencies in the 26 GHz band used for the first time in this test, it is possible to surf the Internet at lightning speed with several gigabits per second. Photo: Christian Charisius/dpa、クレジット：ＤＰＡ／共同通信イメージズ

商品コード: 2019020827399

2019年02月07日

5G technology

07 February 2019, Hamburg: An antenna receiving unit with 5G modem (Fixed Wireless Access FWA) stands next to a laptop on which a speed test indicates a download rate of 1.03 Gigabit per second (Gbps). Shortly before the completion of a test of high-speed Internet connections based on 5G technology in Hamburg, Telefónica Germany has drawn a positive interim balance. With 5G frequencies in the 26 GHz band used for the first time in this test, it is possible to surf the Internet at lightning speed with several gigabits per second. Photo: Christian Charisius/dpa、クレジット：ＤＰＡ／共同通信イメージズ

商品コード: 2019030300731

2019年02月07日

5G technology

07 February 2019, Hamburg: A fiber optic fed antenna unit for 5G is mounted on a roof. Shortly before the completion of a test of high-speed Internet connections based on 5G technology in Hamburg, Telefónica Germany has drawn a positive interim balance. With 5G frequencies in the 26 GHz band used for the first time in this test, it is possible to surf the Internet at lightning speed with several gigabits per second. Photo: Christian Charisius/dpa、クレジット：ＤＰＡ／共同通信イメージズ

商品コード: 2019030300362

2019年02月07日

5G technology

07 February 2019, Hamburg: An antenna receiving unit with 5G modem (Fixed Wireless Access FWA) stands next to a laptop on which a speed test indicates a download rate of 1.01 Gigabit per second (Gbps). Shortly before the completion of a test of high-speed Internet connections based on 5G technology in Hamburg, Telefónica Germany has drawn a positive interim balance. With 5G frequencies in the 26 GHz band used for the first time in this test, it is possible to surf the Internet at lightning speed with several gigabits per second. Photo: Christian Charisius/dpa、クレジット：ＤＰＡ／共同通信イメージズ

商品コード: 2019030300514

2019年02月07日

5G technology

07 February 2019, Hamburg: A fiber optic fed antenna unit for 5G is mounted on a roof. Shortly before the completion of a test of high-speed Internet connections based on 5G technology in Hamburg, Telefónica Germany has drawn a positive interim balance. With 5G frequencies in the 26 GHz band used for the first time in this test, it is possible to surf the Internet at lightning speed with several gigabits per second. Photo: Christian Charisius/dpa、クレジット：ＤＰＡ／共同通信イメージズ

商品コード: 2019030300513

2019年02月07日

5G technology

07 February 2019, Hamburg: A fiber optic fed antenna unit for 5G is mounted on a roof. Shortly before the completion of a test of high-speed Internet connections based on 5G technology in Hamburg, Telefónica Germany has drawn a positive interim balance. With 5G frequencies in the 26 GHz band used for the first time in this test, it is possible to surf the Internet at lightning speed with several gigabits per second. Photo: Christian Charisius/dpa、クレジット：ＤＰＡ／共同通信イメージズ

商品コード: 2019030300849

2019年02月07日

5G technology

07 February 2019, Hamburg: A fiber optic fed antenna unit for 5G is mounted on a roof. Shortly before the completion of a test of high-speed Internet connections based on 5G technology in Hamburg, Telefónica Germany has drawn a positive interim balance. With 5G frequencies in the 26 GHz band used for the first time in this test, it is possible to surf the Internet at lightning speed with several gigabits per second. Photo: Christian Charisius/dpa、クレジット：ＤＰＡ／共同通信イメージズ

商品コード: 2019030300701

2019年02月07日

Press conference 5G Internet supply

07 February 2019, Hamburg: An antenna receiving unit with 5G modem (Fixed Wireless Access FWA) stands next to a laptop on which a speed test indicates a download rate of 1.00 Gigabit per second (Gbps). Shortly before the completion of a test of high-speed Internet connections based on 5G technology in Hamburg, Telefónica Germany has drawn a positive interim balance. With 5G frequencies in the 26 GHz band used for the first time in this test, it is possible to surf the Internet at lightning speed with several gigabits per second. Photo: Christian Charisius/dpa、クレジット：ＤＰＡ／共同通信イメージズ

商品コード: 2019020827211

2019年02月07日

Press conference 5G Internet supply

07 February 2019, Hamburg: An antenna receiving unit with 5G modem (Fixed Wireless Access FWA) stands next to a laptop on which a speed test indicates a download rate of 1.00 Gigabit per second (Gbps). Shortly before the completion of a test of high-speed Internet connections based on 5G technology in Hamburg, Telefónica Germany has drawn a positive interim balance. With 5G frequencies in the 26 GHz band used for the first time in this test, it is possible to surf the Internet at lightning speed with several gigabits per second. Photo: Christian Charisius/dpa、クレジット：ＤＰＡ／共同通信イメージズ

商品コード: 2019020827221

2019年02月07日

Press conference 5G Internet supply

07 February 2019, Hamburg: An antenna receiving unit with 5G modem (Fixed Wireless Access FWA) stands next to a laptop on which a speed test indicates a download rate of 1.02 Gigabit per second (Gbps). Shortly before the completion of a test of high-speed Internet connections based on 5G technology in Hamburg, Telefónica Germany has drawn a positive interim balance. With 5G frequencies in the 26 GHz band used for the first time in this test, it is possible to surf the Internet at lightning speed with several gigabits per second. Photo: Christian Charisius/dpa、クレジット：ＤＰＡ／共同通信イメージズ

商品コード: 2019020827210

2019年02月07日

Press conference 5G Internet supply

07 February 2019, Hamburg: A fiber optic fed antenna unit for 5G is mounted on a roof. Shortly before the completion of a test of high-speed Internet connections based on 5G technology in Hamburg, Telefónica Germany has drawn a positive interim balance. With 5G frequencies in the 26 GHz band used for the first time in this test, it is possible to surf the Internet at lightning speed with several gigabits per second. Photo: Christian Charisius/dpa、クレジット：ＤＰＡ／共同通信イメージズ

商品コード: 2019020827318

2019年02月07日

5G technology

07 February 2019, Hamburg: A fiber optic fed antenna unit for 5G is mounted on a roof. Shortly before the completion of a test of high-speed Internet connections based on 5G technology in Hamburg, Telefónica Germany has drawn a positive interim balance. With 5G frequencies in the 26 GHz band used for the first time in this test, it is possible to surf the Internet at lightning speed with several gigabits per second. Photo: Christian Charisius/dpa、クレジット：ＤＰＡ／共同通信イメージズ

商品コード: 2019030300850

2019年02月07日

Press conference 5G Internet supply

07 February 2019, Hamburg: A fiber optic fed antenna unit for 5G is mounted on a roof. Shortly before the completion of a test of high-speed Internet connections based on 5G technology in Hamburg, Telefónica Germany has drawn a positive interim balance. With 5G frequencies in the 26 GHz band used for the first time in this test, it is possible to surf the Internet at lightning speed with several gigabits per second. Photo: Christian Charisius/dpa、クレジット：ＤＰＡ／共同通信イメージズ

商品コード: 2019020827417

01:23.49

2019年02月12日

「新華社」重慶市にスマート駐車場、都心部の駐車難を解消

中国重慶市の九竜坡区は交通量が多く、新たな建設用地にも事欠く中心市街にある。その九竜坡区で新たに建設されたスマート駐車場ビルは、近隣の駐車場不足の解消だけでなく、旧市街で土地資源を節約しつつ駐車場を増やす上で参考となるプランを示した。建設されたスマート駐車場ビルは２２階建てで、敷地面積は６８０平方メートルに過ぎないが３８７台を収容できる。必要な土地は従来の駐車場の５分の１ですむ。ビルは古いマンション跡地に建てられており、地形の制約も大きかったため、中国で初めて四角と円形のタワーを組み合わせた設計案を採用。空間利用の最大化を実現した。スマート化システムにより、利用者は便利かつ迅速に車の出し入れができ、手動操作の必要もない。ビルには１４カ所の出入口が設置されており、車が出入口に来るとゲートが自動的に開く。利用者は車をゲート内の駐車スペースに停めるだけで車庫から出ることができ、出入口にある二次元バーコードを携帯で読み取れば自動で入庫が始まる。車を取り出す時には、二次元バーコードを読み取り決済を済ませれば、車が自動的に降りてきて１階のゲート内駐車スペースに戻される。また、車は外向きに置かれ利用者が出庫しやすいようになっている。駐車場ビル内部では、車両用エレベーターが毎秒２・５メートルの速さで動いており、入庫も出庫も９０秒以内で完了できる。（記者／谷訓）＜映像内容＞中国のスマート駐車場の様子、撮影日：撮影日不明、クレジット：新華社／共同通信イメージズ

商品コード: 2019021218320

2019年03月11日

Consequences of night wind storm Eberhard in the Czech Republic

Consequences of night wind storm in the Czech Republic. The national power utility CEZ declared calamity in its whole distribution network in the Czech Republic due to strong wind during the night in Czech Republic, March 11, 2019. Atop the highest Czech mountain, Snezka (1602 metres), the hurricane was travelling at the speed of 57 metres per second (206.6 km/h) at three oｴclock this early morning. (CTK Photo/Vaclav Salek)、クレジット：ＣＴＫ／共同通信イメージズ

商品コード: 2019031300546

2019年03月11日

Consequences of night wind storm Eberhard in the Czech Republic

Consequences of night wind storm in the Czech Republic. The national power utility CEZ declared calamity in its whole distribution network in the Czech Republic due to strong wind during the night in Czech Republic, March 11, 2019. Atop the highest Czech mountain, Snezka (1602 metres), the hurricane was travelling at the speed of 57 metres per second (206.6 km/h) at three oｴclock this early morning. (CTK Photo/Vaclav Salek)、クレジット：ＣＴＫ／共同通信イメージズ

商品コード: 2019031300544

2019年03月11日

Consequences of night wind storm Eberhard in the Czech Republic, Train station Olomouc, delay

Consequences of night wind storm in the Czech Republic. The national power utility CEZ declared calamity in its whole distribution network in the Czech Republic due to strong wind during the night in Czech Republic, March 11, 2019. Atop the highest Czech mountain, Snezka (1602 metres), the hurricane was travelling at the speed of 57 metres per second (206.6 km/h) at three oｴclock this early morning. (CTK Photo/Ludek Perina)、クレジット：ＣＴＫ／共同通信イメージズ

商品コード: 2019031300605

2019年03月11日

Consequences of night wind storm Eberhard in the Czech Republic

Consequences of night wind storm in the Czech Republic. The national power utility CEZ declared calamity in its whole distribution netwrok in the Czech Republic due to strong wind during the night in Czech Republic, March 11, 2019. Atop the highest Czech mountain, Snezka (1602 metres), the hurricane was travelling at the speed of 57 metres per second (206.6 km/h) at three oｴclock this early morning. (CTK Photo/Libor Zavoral)、クレジット：ＣＴＫ／共同通信イメージズ

商品コード: 2019031300616

2019年03月11日

Consequences of night wind storm Eberhard in the Czech Republic

Consequences of night wind storm in the Czech Republic. The national power utility CEZ declared calamity in its whole distribution network in the Czech Republic due to strong wind during the night in Czech Republic, March 11, 2019. Atop the highest Czech mountain, Snezka (1602 metres), the hurricane was travelling at the speed of 57 metres per second (206.6 km/h) at three oｴclock this early morning. (CTK Photo/Vaclav Salek)、クレジット：ＣＴＫ／共同通信イメージズ

商品コード: 2019031300549

2019年03月11日

Consequences of night wind storm Eberhard in the Czech Republic

Consequences of night wind storm in the Czech Republic. The national power utility CEZ declared calamity in its whole distribution network in the Czech Republic due to strong wind during the night in Czech Republic, March 11, 2019. Atop the highest Czech mountain, Snezka (1602 metres), the hurricane was travelling at the speed of 57 metres per second (206.6 km/h) at three oｴclock this early morning. (CTK Photo/Vaclav Salek)、クレジット：ＣＴＫ／共同通信イメージズ

商品コード: 2019031300557

2019年03月11日

Consequences of night wind storm Eberhard in the Czech Republic

Consequences of night wind storm in the Czech Republic. The national power utility CEZ declared calamity in its whole distribution network in the Czech Republic due to strong wind during the night in Czech Republic, March 11, 2019. Atop the highest Czech mountain, Snezka (1602 metres), the hurricane was travelling at the speed of 57 metres per second (206.6 km/h) at three oｴclock this early morning. (CTK Photo/Josef Vostarek)、クレジット：ＣＴＫ／共同通信イメージズ

商品コード: 2019031300676

2019年03月11日

Consequences of night wind storm Eberhard in the Czech Republic

Consequences of night wind storm in the Czech Republic. The national power utility CEZ declared calamity in its whole distribution network in the Czech Republic due to strong wind during the night in Czech Republic, March 11, 2019. Atop the highest Czech mountain, Snezka (1602 metres), the hurricane was travelling at the speed of 57 metres per second (206.6 km/h) at three oｴclock this early morning. (CTK Photo/Vaclav Salek)、クレジット：ＣＴＫ／共同通信イメージズ

商品コード: 2019031300687

2019年03月11日

Consequences of night wind storm Eberhard in the Czech Republic

Consequences of night wind storm in the Czech Republic. The national power utility CEZ declared calamity in its whole distribution network in the Czech Republic due to strong wind during the night in Czech Republic, March 11, 2019. Atop the highest Czech mountain, Snezka (1602 metres), the hurricane was travelling at the speed of 57 metres per second (206.6 km/h) at three oｴclock this early morning. (CTK Photo/Vaclav Pancer)、クレジット：ＣＴＫ／共同通信イメージズ

商品コード: 2019031300706

2019年03月11日

Consequences of night wind storm Eberhard in the Czech Republic, fallen tree

Consequences of night wind storm in the Czech Republic. The national power utility CEZ declared calamity in its whole distribution network in the Czech Republic due to strong wind during the night in Czech Republic, March 11, 2019. Atop the highest Czech mountain, Snezka (1602 metres), the hurricane was travelling at the speed of 57 metres per second (206.6 km/h) at three oｴclock this early morning. (CTK Photo/Radek Petrasek)、クレジット：ＣＴＫ／共同通信イメージズ

商品コード: 2019031300594

2019年03月11日

Consequences of night wind storm Eberhard in the Czech Republic

Consequences of night wind storm in the Czech Republic. The national power utility CEZ declared calamity in its whole distribution network in the Czech Republic due to strong wind during the night in Czech Republic, March 11, 2019. Atop the highest Czech mountain, Snezka (1602 metres), the hurricane was travelling at the speed of 57 metres per second (206.6 km/h) at three oｴclock this early morning. (CTK Photo/David Tanecek)、クレジット：ＣＴＫ／共同通信イメージズ

商品コード: 2019031300584

2019年03月11日

Consequences of night wind storm Eberhard in the Czech Republic

Consequences of night wind storm in the Czech Republic. The national power utility CEZ declared calamity in its whole distribution network in the Czech Republic due to strong wind during the night in Czech Republic, March 11, 2019. Atop the highest Czech mountain, Snezka (1602 metres), the hurricane was travelling at the speed of 57 metres per second (206.6 km/h) at three oｴclock this early morning. (CTK Photo/Vaclav Salek)、クレジット：ＣＴＫ／共同通信イメージズ

商品コード: 2019031300562

2019年03月11日

Consequences of night wind storm Eberhard in the Czech Republic

Consequences of night wind storm in the Czech Republic. The national power utility CEZ declared calamity in its whole distribution netwrok in the Czech Republic due to strong wind during the night in Czech Republic, March 11, 2019. Atop the highest Czech mountain, Snezka (1602 metres), the hurricane was travelling at the speed of 57 metres per second (206.6 km/h) at three oｴclock this early morning. (CTK Photo/Libor Zavoral)、クレジット：ＣＴＫ／共同通信イメージズ

商品コード: 2019031300572

2019年03月11日

Consequences of night wind storm Eberhard in the Czech Republic

Consequences of night wind storm in the Czech Republic. The national power utility CEZ declared calamity in its whole distribution network in the Czech Republic due to strong wind during the night in Czech Republic, March 11, 2019. Atop the highest Czech mountain, Snezka (1602 metres), the hurricane was travelling at the speed of 57 metres per second (206.6 km/h) at three oｴclock this early morning. (CTK Photo/David Tanecek)、クレジット：ＣＴＫ／共同通信イメージズ

商品コード: 2019031300503

2019年03月11日

Consequences of night wind storm Eberhard in the Czech Republic

Consequences of night wind storm in the Czech Republic. The national power utility CEZ declared calamity in its whole distribution network in the Czech Republic due to strong wind during the night in Czech Republic, March 11, 2019. Atop the highest Czech mountain, Snezka (1602 metres), the hurricane was travelling at the speed of 57 metres per second (206.6 km/h) at three oｴclock this early morning. (CTK Photo/David Tanecek)、クレジット：ＣＴＫ／共同通信イメージズ

商品コード: 2019031300588

2019年03月11日

Consequences of night wind storm Eberhard in the Czech Republic

Consequences of night wind storm in the Czech Republic. The national power utility CEZ declared calamity in its whole distribution netwrok in the Czech Republic due to strong wind during the night in Czech Republic, March 11, 2019. Atop the highest Czech mountain, Snezka (1602 metres), the hurricane was travelling at the speed of 57 metres per second (206.6 km/h) at three oｴclock this early morning. (CTK Photo/Libor Zavoral)、クレジット：ＣＴＫ／共同通信イメージズ

商品コード: 2019031300563

2019年03月11日

Consequences of night wind storm Eberhard in the Czech Republic, Dobrenice

Consequences of night wind storm in the Czech Republic. The national power utility CEZ declared calamity in its whole distribution network in the Czech Republic due to strong wind during the night in Czech Republic, March 11, 2019. Atop the highest Czech mountain, Snezka (1602 metres), the hurricane was travelling at the speed of 57 metres per second (206.6 km/h) at three oｴclock this early morning. (CTK Photo/David Tanecek)、クレジット：ＣＴＫ／共同通信イメージズ

商品コード: 2019031300579

2019年03月11日

Consequences of night wind storm Eberhard in the Czech Republic

Consequences of night wind storm in the Czech Republic. The national power utility CEZ declared calamity in its whole distribution network in the Czech Republic due to strong wind during the night in Czech Republic, March 11, 2019. Atop the highest Czech mountain, Snezka (1602 metres), the hurricane was travelling at the speed of 57 metres per second (206.6 km/h) at three oｴclock this early morning. (CTK Photo/Vaclav Pancer)、クレジット：ＣＴＫ／共同通信イメージズ

商品コード: 2019031300698

報道写真の購入なら共同通信イメージリンク

「毎秒」の写真・グラフィックス・映像