磁場の写真・画像 : 報道写真・ニュース映像ならKYODO NEWS IMAGELINK(イメージリンク)

-

Sunspot Up Close.

Sunspot Up Close. The Sun‘s complex magnetic field creates this cool region by inhibiting hot material from entering the spot. Sunspots can be larger than the Earth and typically last for only a few days. This high-resolution picture also shows clearly that the Sun‘s face is a bubbling sea of separate cells of hot gas. These cells are known as granules. A solar granule is about 1000 kilometres across and lasts about 10 minutes. After that, many granules end up exploding.、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: 2019022103717

-

Sunspot with streamers of super-hot

Sunspot with streamers of super-hot, electrically charged gas (plasma) arc from the surface of the Sun, revealing the structure of the solar magnetic field. Credit NASA.、クレジット：ＮＡＳＡ／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: 2019022103722

-

Joseph Wilson Swan (1828-1914) British physicist and chemist.

Joseph Wilson Swan (1828-1914) British physicist and chemist. Photography (bromide paper): Incandescent light bulb. Here a Royal Society Conversazione, 8 May 1889, demonstrating that metal ring wound with coil of wire rotates in Earth‘s magnetic field when small current applied. 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: 2019082902359

1904年12月31日

Apparatus used by the Curies to investigate the deflection of the beta rays from radium

Apparatus used by the Curies to investigate the deflection of the beta rays from radium (R) in magnetic field. Engraving published Paris 1904、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: 2019073103073

1963年05月31日

阪大、プラズマ閉じ込め装置

公開された大阪大学工学部超高温工学研究室の「カスプ磁場プラズマ閉じ込め装置」＝１９６３（昭和３８）年５月３１日、大阪府枚方市

商品コード: 2011072600231

1963年09月09日

Kurchatov Institute of Atomic Energy

09.09.1963 The Kurchatov Institute of Atomic Energy, now the Kurchatov Institute. Photo: An upgraded PR-5 adiabatic trap with a combined magnetic field, developed by a team of Russian physicists. Dmitriy Kozlov、クレジット：Ｓｐｕｔｎｉｋ／共同通信イメージズ

商品コード: 2019091101545

1963年09月09日

Kurchatov Institute of Atomic Energy

09.09.1963 Kurchatov Institute of Atomic Energy (now Kurchatov Institute). Soviet scientists Y. Baiborodov, M. Ioffe, V. Petrov and R. Sobolev conduct experiments with the use of the PR-5 unit, an adiabatic trap with the magnetic field increasing both longitudinally and radially. Dmitriy Kozlov、クレジット：Ｓｐｕｔｎｉｋ／共同通信イメージズ

商品コード: 2019091201675

1965年07月01日

Sailing-motor schooner Zarya on Neva River

01.07.1965 The three-mast sailing-motor schooner Zarya on Neva River in the city of Leningrad. The ship was built in Finland in the shipyard of the port of Turku in 1952 at the order from the Academy of Sciences of the USSR. Zarya is the world‘s only non-magnetic vessel used to study Earth‘s magnetic field, with scientists of the Academy‘s Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation involved in the work. Boris Losin、クレジット：Ｓｐｕｔｎｉｋ／共同通信イメージズ

商品コード: 2019100802563

1966年06月15日

Zarya sailing-motor schoone

15.06.1966 Latvian SSR. Non-magnetic sailing-motor schoone Zarya (Soviet scientific-research vessel for studying the Earth‘s magnetic field) in the Port of Liepaja.、クレジット：Ｓｐｕｔｎｉｋ／共同通信イメージズ

商品コード: 2019052704314

1967年09月01日

MAGNETOLOGIST ANTARCTICA

01.09.1967 A magnetologist measuring the magnetic field inside an ice tunnel in Antarctica. G. Koposov / Sputnik、クレジット：Ｓｐｕｔｎｉｋ／共同通信イメージズ

商品コード: 2022111602297

1969年11月04日

Joint Institute for Nuclear Research

5720448 04.11.1969 Joint Institute for Nuclear Research in Dubna. Proton synchrotron accelerator in the high energies‘ laboratory. Georgij、クレジット：Ｓｐｕｔｎｉｋ／共同通信イメージズ

商品コード: 2022071108967

1974年11月15日

阪大核物理研センター完成

完成した大阪大学核物理研究センターの高性能サイクロトロン（イオン加速装置）。日本初の大型ＡＶＦ（周回方向変動磁場）型サイクロトロンと呼ばれ、陽子や重陽子などの軽いイオンの加速には非常に有効な加速器＝１９７４（昭和４９）年１１月１５日、大阪府吹田市

商品コード: 2012052800132

1976年07月16日

名大プラズマ研究所プラズマ発生装置を試運転

試運転が始まった環状磁場系プラズマ発生装置「ＪＩＰＰ・Ｔ－ＩＩ」。プラズマの青白い光がテレビの画面に－「人工太陽」と呼ばれる核融合炉の実現に向けて名古屋大学プラズマ研究所で実験装置の試運転が始まった＝１９７６（昭和５１）年７月１６日、名古屋市千種区

商品コード: 2013112100121

1978年01月29日

磁場コイル核融合臨界装置、日立に発注

日立が試作した「ＪＴ６０」用のトロイダル磁場コイル

商品コード: 2015032400267

1978年12月23日

Leipunsky Institute of Physics and Power Engineering

8147014 22.12.1978 The Leipunsky Institute of Physics and Power Engineering, now the Leipunsky National Research Center / Institute of Physics and Power Engineering. Photo: Nuclear physicists stand near a cyclotron, a unit for the cyclic acceleration of charged particles inside a magnetic field. Oleg Kuzmin、クレジット：Ｓｐｕｔｎｉｋ／共同通信イメージズ

商品コード: 2022040211795

1989年01月23日

MAGNETIC FIELD ELECTRON STREAM TOKAMAK-15

151317 23.01.1989 The Tokamak-15 thermonuclear facility at the Kurchatov Atomic Energy Institute. An electron stream (the bright horizontal line) along a magnetic field line. Prihodko / Sputnik、クレジット：Ｓｐｕｔｎｉｋ／共同通信イメージズ

商品コード: 2022052111377

1989年06月17日

「宙に浮くはさみ」輪切り、縦切り自由自在

（４）「宙に浮くはさみ」ＭＲＩ近くで発生する強力な磁力線は地球磁場の約５万倍。ひもでつるした鉄のはさみは宙に浮いたまま＝京都府船井郡日吉町の明治鍼灸大付属病院

商品コード: 2019122500519

1990年04月24日

Ultraviolet image of an electric-blue aurora glowing on the giant planet Jupiter

Hubble Space Telescope, ultraviolet image of an electric-blue aurora glowing on the giant planet Jupiter. Auroras are curtains of light resulting from high-energy electrons racing along the planet‘s magnetic field into the upper atmosphere. The electrons excite atmospheric gases, causing them to glow. The image shows the main oval of the aurora, which is cantered on the magnetic north pole, plus more diffuse emissions inside the polar cap. Though the aurora resembles the same phenomenon that crowns Earth‘s polar regions, the Hubble image shows unique emissions from the magnetic ‘footprints‘ of three of Jupiter‘s largest moons. Auroral footprints can be seen in this image from Io (along the left-hand limb), Ganymede (near the centre), and Europa (just below and to the right of Ganymede‘s Auroral footprint). 、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: 2018111215800

1992年12月31日

Artist‘s concept of the pulsar planet system discovered by Aleksander Wolszczan in 1992.

Artist‘s concept of the pulsar planet system discovered by Aleksander Wolszczan in 1992. Wolszczan used the Arecibo radio telescope in Puerto Rico to find three planets - the first of any kind ever found outside our solar system - circling a pulsar called PSR B1257+12. Pulsars are rapidly rotating neutron stars, which are the collapsed cores of exploded massive stars. They spin and pulse with radiation, much like a lighthouse beacon. Here, the pulsar‘s twisted magnetic fields are highlighted by the blue glow.、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: 2019091002643

1995年04月25日

磁場がないと一瞬広がり微小重力でも炎燃え続ける

磁場がない微小重力下では炎は一瞬広がり、すぐ消えてしまう（カラーネガ）

商品コード: 1995042500078

1995年04月25日

磁場がないと一瞬広がり微小重力でも炎燃え続ける

磁場がない微小重力下では炎は一瞬広がり、すぐ消えてしまう（カラーネガ）

商品コード: 1995042500074

1995年04月25日

磁場をかけて燃える微小重力でも炎燃え続ける

微小重力下でも磁場をかけると、酸素の対流が発生し、炎は明るく燃え続ける（カラーネガ）

商品コード: 1995042500077

1995年04月25日

磁場をかけて燃える微小重力でも炎燃え続ける

微小重力下でも磁場をかけると、酸素の対流が発生し、炎は明るく燃え続ける（カラーネガ）（北海道上砂川町の「地下無重力実験センター」で実験した）

商品コード: 1995042500075

1995年06月24日

コンピューターアニメユリシーズ、太陽の両極に

米航空宇宙局（ＮＡＳＡ）と欧州宇宙機関（ＥＳＡ）が共同開発し、１９９０年１０月に打ち上げた太陽探査機「ユリシーズ」が昨年９月、太陽の南極上空を飛行した際の様子を描いたコンピューターアニメ（想像図）。ユリシーズは太陽の両極の太陽風や磁場を観測する初の探査機で、今年７月３１日にはいよいよ北極点の上空に到達する。（ロイター＝共同）

商品コード: 1995062400033

1995年06月24日

コンピューターアニメユリシーズ、太陽の両極に

米航空宇宙局（ＮＡＳＡ）と欧州宇宙機関（ＥＳＡ）が共同開発し、１９９０年１０月に打ち上げた太陽探査機「ユリシーズ」が昨年９月、太陽の南極上空を飛行した際の様子を描いたコンピューターアニメ（想像図）。ユリシーズは太陽の両極の太陽風や磁場を観測する初の探査機で、今年７月３１日にはいよいよ北極点の上空に到達する。（ロイター＝共同）

商品コード: 1995062400034

1997年12月22日

辻尚子さん

インドには聖地の磁場があると話す辻尚子さん（画家・つじたかこ）

商品コード: 1997122200033

1998年09月14日

みはし・まりさん

沖縄には磁場のようなものを感じると話すみはし・まりさん

商品コード: 1998091400098

1999年12月08日

浮いたガラス強磁場無重力でガラス溶解

強磁場発生装置内の疑似無重力状態で浮いたガラス

商品コード: 1999120800026

1999年12月08日

真球になったガラス強磁場無重力でガラス溶解

強磁場発生装置内の疑似無重力状態で溶解し真球になったガラス

商品コード: 1999120800025

2001年02月28日

回転磁場発生装置がん組織内を動いて治療

マイクロマシンにかける回転磁場発生装置を調整する東北大電気通信研究所の石山和志助手＝６日、仙台市青葉区の同研究所

商品コード: 2001022800008

2001年02月28日

マイクロマシンがん組織内を動いて治療

周囲から加えられた磁場で、回転しながら寒天の中を進み先端が飛び出したマイクロマシン（１目盛りは５ミリ）＝６日、仙台市青葉区の東北大電気通信研究所

商品コード: 2001022800007

2002年03月22日

岡田主任研究員新超電導物質の線材で磁場

日立製作所などが作製した二ホウ化マグネシウムの線材を持つ岡田道哉主任研究員＝２２日、東京都千代田区の日立製作所本社

商品コード: 2002032200150

2004年06月01日

日立が開発した心磁計磁場で心疾患を早期発見

日立製作所が開発した移動可能な心臓磁場計測装置

商品コード: 2004060100960

2005年06月13日

地域に生まれる文化の磁場

小島多恵子さん

商品コード: 2005061300075

2009年09月22日

日本総研の寺島会長北ヤード「情報の磁場」に

インタビューに答える日本総合研究所の寺島実郎会長

商品コード: 2009092200085

2009年09月22日

北ヤード「情報の磁場」に

大阪・梅田北ヤード再開発地域

商品コード: 2009092200089

2009年09月22日

北ヤード「情報の磁場」に

大阪・梅田北ヤード再開発地域

商品コード: 2009092200090

2009年09月22日

北ヤード「情報の磁場」に

大阪・梅田北ヤード再開発地域

商品コード: 2009092200091

2009年09月22日

北ヤード「情報の磁場」に

大阪・梅田北ヤード再開発地域

商品コード: 2009092200092

2013年09月11日

氷床の増減、磁場にも影響

地球磁場が変動する仕組み

商品コード: 2013091100032

2013年09月11日

氷床の増減、磁場にも影響

地球磁場が変動する仕組み

商品コード: 2013091100035

2013年10月10日

公開された試作部品ＩＴＥＲ主要部品を受注

三菱重工業が製作を始めた「トロイダル磁場コイル」の試作部品の一部＝１０日午後、兵庫県明石市

商品コード: 2013101000474

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

00:19.86

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

00:33.43

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

00:13.20

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

00:23.83

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

00:15.70

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

00:17.33

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

00:22.26

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

00:12.66

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

00:20.13

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

00:20.53

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

00:16.93

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

00:19.46

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

00:11.20

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

00:17.66

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

00:16.53

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

00:27.26

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

00:30.96

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

00:33.10

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

00:28.06

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

00:16.78

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

2014年05月20日

公開された大型コンデンサー国内最大の充電システム

大阪大の先端強磁場科学研究センターで公開された、瞬間的に強い磁場を発生させる大型コンデンサーバンクシステム＝２０日午後、大阪府豊中市

商品コード: 2014052000671

2014年05月20日

大阪大の充電システム国内最大の充電システム

大阪大の先端強磁場科学研究センターで公開された、充電量が国内最大の大型コンデンサーバンクシステム＝２０日午後、大阪府豊中市

商品コード: 2014052000672

2014年10月28日

ＭＲＩの手術室システム高磁場ＭＲＩ備えた手術室

国内で初めて稼働する、京都大病院の高磁場のＭＲＩ（左奥）を備えた手術室システム＝２８日、京都市

商品コード: 2014102800626

2017年02月22日

地球の磁場、誕生直後から

地球の核の対流

商品コード: 2017022200901

2017年02月22日

地球の磁場、誕生直後から

地球の核の対流

商品コード: 2017022200902

2017年05月17日

分杭峠

キーワード：屋外、自然、春、昼、日本、風景、無人、分杭峠、パワースポット、ゼロ磁場、風景メイン写真＝２０１７（平成２９）年５月１７日、長野県伊那市、クレジット：ＴＡＤＡＯ　ＹＡＭＡＭＯＴＯ／ａ．ｃｏｌｌｅｃｔｉｏｎＲＦ／アマナイメージズ／共同通信イメージズ

商品コード: 2020062904610

00:19.68

2017年12月04日

Aurora borealis and weather station

Timelapse footage of aurora borealis lighting the sky above two photographers and a weather station. The aurora borealis, or northern lights, are formed when charged particles in the solar wind are attracted to the Earth‘s poles by its magnetic field. The particles collide with gas molecules in the upper atmosphere, ionising them, and they emit light as they recombine. Filmed by Hornsund fjord, in southern Spitsbergen, Norway.、クレジット：ＫＲＺＹＳＺＴＯＦ　ＧＲＡＢＩＥＣ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022061405891

00:06.00

2017年12月04日

Aurora borealis, timelapse

Timelapse footage of the aurora borealis in the night sky. The aurora are caused when charged particles in the solar wind are channeled to the poles by the Earth‘s magnetic field. Here they collide with gases in the atmosphere, exciting them. The gases emit light when they return to a non-excited state. Filmed from Spitsbergen island in the Norwegian Arctic.、クレジット：ＫＲＺＹＳＺＴＯＦ　ＧＲＡＢＩＥＣ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022061405876

00:24.93

2017年12月04日

Aurora borealis, timelapse

Timelapse footage of the aurora borealis in the night sky. The aurora are caused when charged particles in the solar wind are channeled to the poles by the Earth‘s magnetic field. Here they collide with gases in the atmosphere, exciting them. The gases emit light when they return to a non-excited state. Filmed from Spitsbergen island in the Norwegian Arctic.、クレジット：ＫＲＺＹＳＺＴＯＦ　ＧＲＡＢＩＥＣ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022061405896

00:07.76

2017年12月04日

Aurora borealis, timelapse

Timelapse footage of the aurora borealis in the night sky. The aurora are caused when charged particles in the solar wind are channeled to the poles by the Earth‘s magnetic field. Here they collide with gases in the atmosphere, exciting them. The gases emit light when they return to a non-excited state. Filmed from Spitsbergen island in the Norwegian Arctic.、クレジット：ＫＲＺＹＳＺＴＯＦ　ＧＲＡＢＩＥＣ／ＳＣＩＥＮＣＥ　ＰＨＯＴＯ　ＬＩＢＲＡＲＹ／共同通信イメージズ

商品コード: 2022061405883

2018年10月28日

NASA Spacecraft ‘Touches‘ The Sun For First Time

December 15, 2021: Illustration of Parker Solar Probe approaching the Sun. For the first time in history, a spacecraft has “touched“ the sun, scientists announced. NASA‘s Parker Solar Probe has flown through the sun‘s upper atmosphere, the corona, and sampled particles and magnetic fields there. The news was announced during a meeting of the American Geophysical Union. Parker Solar Probe launched in 2018 to explore the mysteries of the sun by traveling closer to it than any spacecraft before. Three years after launch and decades after first conception, Parker has finally arrived. (Credit Image: © APL/NASA/ZUMA Wire)、クレジット：©ＡＰＬ／ＮＡＳＡ／ＺＵＭＡ　Ｗｉｒｅ／共同通信イメージズ

商品コード: 2021121606257

02:03.71

2019年06月04日

「新華社」百年の屋敷が伝える家風、文化観光の新たな目玉に

中国江西省南昌市北部郊外の新建区に、歴史的建築物が立ち並ぶ「汪山土庫（おうさんどこ）」がある。この屋敷群に代々伝わる優れた家風が独特の「磁場」を形作り、每月万単位の観光客を引き寄せている。汪山土庫は新建程氏一族の居住地で、南昌市北部郊外の新建区大塘坪郷汪山崗に位置し、１０８ムー（約７ヘクタール）の敷地内に２５棟の家屋が建ち、部屋数は全部で１４４３部屋、５７２の中庭がある。ここ２００年の間に、汪山土庫からは百人以上に上る社会各界の著名人が輩出しており、輝かしい知の流れを脈々と伝えてきた。この５年間で汪山土庫の主だった建物が修理され、各種インフラ設備も日に日に整い、延べ３０万人余りの観光客を迎えてきた。その名を慕って訪れ、程氏一族の物語に耳を傾ける人々がますます増えている。観光客を相手に昔の物語を語る合間を縫っては、程さんは小学校入学を控えた孫に「程氏家訓十条」の音読指導をしている。程氏一族の人々は現在、世界３１の国や地域に散らばっている。郷里に残った一人として、程さんはこの先も生家を守り続け、より多くの観光客に自らよき家風を伝えていくつもりだ。（記者／黄浩然）＜映像内容＞「汪山土庫」の街並みなど風景、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: 2019060404900

2019年07月12日

天王星天王・海王星の強磁場解明

無人惑星探査機ボイジャー２号が１９８６年に撮影した天王星（ＮＡＳＡ提供・共同）

商品コード: 2019071201767

2019年09月09日

NASA Unveil New Image Of Tycho Supernova ‘Seen By Shakespeare‘

September 9, 2019, United States: This image shows: Using data from NASAÃ¢â¬â¢s Imaging X-ray Polarimetry Explorer (IXPE), international researchers have uncovered new information about the Tycho supernova remnant, an exploded star in the constellation Cassiopeia, the light from which was first seen on Earth in 1572. The results offer new clues about how shock waves created by these titanic stellar explosions accelerate particles to nearly the speed of light, and reveal, for the first time, the geometry of the magnetic fields close to the supernovaÃ¢â¬â¢s blast wave, which forms a boundary around the ejected material, as seen in this composite image. IXPE data (dark purple and white) have been combined with data from NASAÃ¢â¬â¢s Chandra X-ray Observatory (red and blue) and overlaid with the stars in the field of view as captured by the Digitized Sky Survey....An international team of scientists has uncovered new information about the remains of a star whose explosion was discovered 450 years ago - and poss...

商品コード: 2023030204092

2019年12月04日

ピエゾソニックの超音波モーター「ＰＳＭ６０Ｎ―ＥＴ」。モーター（手前）とドライバー（奥）

Ｐｉｅｚｏ　Ｓｏｎｉｃ（ピエゾソニック、東京都世田谷区）は、高トルク超音波モーター「ＰＳＭ６０Ｎ」を発売した。超音波モーターは微小振動と摩擦力で回転する。コイルと磁石を用いないため磁気共鳴断層撮影装置（ＭＲＩ）などの高磁場環境で利用できる。エンコーダー付きのモーターと制御ドライバーのセットで価格は消費税込みで２０万３９４０円。１年間で５００―１０００セットの販売を目指す。同社の超音波モーターは、くし歯状のスリットが入ったリングを圧電素子で振動させる。リングにローター（回転体）を接触させると、くし歯の振動がローターに伝わり回転する。くし歯構造が振動を増幅する。摩擦の大きい材料を選び、トルクを高めた。最大トルクは１・２ニュートンメートルで、同サイズの直流モーターの５―１０倍にあたるという。光学式のエンコーダーも搭載した。＝２０１９（令和元）年１２月４日、撮影場所不明、クレジット：日刊工業新聞／共同通信イメージズ

商品コード: 2019121201187