[]
Your ongoing selection
Asset(s) Assets
Your quote 0

Your selection

Clear selection
Item added to cart
View cart and checkout
{"event":"pageview","page_type1":"undetected","page_type2":"_assets_search_override","language":"en","user_logged":"false","user_type":"ecommerce","nl_subscriber":"false"}
{"event":"ecommerce_event","event_name":"view_item","event_category":"browse_catalog","ecommerce":{"items":[{"item_id":"UIG3480080","item_category":"illustration","item_category2":"out_of_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"corby_browning_s_mircospectroscope_1895","item_variant":"undefined"},{"item_id":"UIG531380","item_category":"illustration","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"electromagnetic_spectrum_the_visible_range_shaded_portion_is_shown_enlarged_on_the_right","item_variant":"undefined"},{"item_id":"PIX4650395","item_category":"illustration","item_category2":"no_copyright","item_category3":"standard","item_category4":"d_ducros","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_electromagnetic_spectrum_electromagnetic_spectrum_artwork_artist_s_view_of_the_different_means_o","item_variant":"undefined"},{"item_id":"UDK844614","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"electromagnetic_spectrum_neon_tube_showing_a_characteristic_orange_glow","item_variant":"undefined"},{"item_id":"UDK844612","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"electromagnetic_spectrum_green_led_light_emitting_diode_showing_a_green_glow","item_variant":"undefined"},{"item_id":"UDK844616","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"green_red_and_blue_coloured_disks_showing_the_subtractive_process_the_three_filters_contain_pigments","item_variant":"undefined"},{"item_id":"PIX4669145","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"earth_seen_by_satellite_dscovr_earth_seen_by_satellite_dscovr_earth_photo_obtained_by_satellite_deep","item_variant":"undefined"},{"item_id":"UIG3480079","item_category":"illustration","item_category2":"out_of_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"hofmann_s_spectroscope_1895","item_variant":"undefined"},{"item_id":"UIS5089695","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"gustav_kirchhoff_german_physicist_c_1860s","item_variant":"undefined"},{"item_id":"UIS5622875","item_category":"illustration","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"gustav_robert_kirchhoff_german_physicist_c_1870s","item_variant":"undefined"},{"item_id":"UIS5071203","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"gustav_robert_kirchhoff_german_physicist_c_1860s","item_variant":"undefined"},{"item_id":"UIS5092777","item_category":"illustration","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"gustav_kirchhoff_german_physicist_mid_19th_century","item_variant":"undefined"},{"item_id":"UIS5070598","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"false_colour_image_of_a_solar_flare_photographed_from_skylab_1973_solar_flares_are_sudden_outbursts_","item_variant":"undefined"},{"item_id":"UIS5070673","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"post_flare_loop_above_the_sun_s_surface_false_colour_photograph_by_skylab_1973","item_variant":"undefined"},{"item_id":"UIS5070694","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"solar_flare_eruption_in_extreme_ultraviolet_light_photographed_from_skylab_1973","item_variant":"undefined"},{"item_id":"UIS5072119","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"false_colour_photograph_of_the_sun_and_the_moon_taken_from_skylab_1970s","item_variant":"undefined"},{"item_id":"UIS5070615","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"large_solar_flare_seen_in_extreme_ultraviolet_light_1973","item_variant":"undefined"},{"item_id":"PIX4625407","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"japet_satellite_of_saturn_seen_by_cassini_crescent_of_iapetus_seen_by_cassini_spacecraft_mosaic_in_f","item_variant":"undefined"},{"item_id":"UIS5070609","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"solar_flare_seen_in_helium_3_light_photographed_from_skylab_1973","item_variant":"undefined"},{"item_id":"UIS5070627","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"post_flare_loop_above_the_sun_s_surface_ultraviolet_photograph_from_skylab_1973","item_variant":"undefined"},{"item_id":"UIS5070631","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"false_colour_image_of_the_solar_corona_photographed_from_skylab_1973","item_variant":"undefined"},{"item_id":"UIS5070626","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"solar_flare_eruption_in_false_colour_photographed_from_skylab_1973","item_variant":"undefined"},{"item_id":"PIX4610559","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"barree_spiral_galaxy_ngc_3259_in_the_great_bear_barred_spiral_galaxy_ngc_3259_in_ursa_major_the_barr","item_variant":"undefined"},{"item_id":"PIX4626499","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"crab_nebula_seen_in_different_wavelength_the_crab_nebula_in_multi_wavelength_m1_the_crab_nebula_is_t","item_variant":"undefined"},{"item_id":"PIX4634312","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"map_of_the_sky_seen_by_planck_the_microwave_sky_as_seen_by_planck_380_000_years_after_the_formation_","item_variant":"undefined"},{"item_id":"PIX4582960","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"remains_of_the_supernova_kepler_in_ophiuchus_nasa_s_three_great_observatories_the_hubble_space_teles","item_variant":"undefined"}]}}
{"event":"custom_event","event_name":"view_search_result","event_category":"browse_catalog","keyword":"electromagnetic spectrum","search_type":"standard","search_bridgeman_artists":"false","search_mode":"automatic","search_zero_result":"false","search_results":26,"search_results_page_number":1}

'Electromagnetic Spectrum' images and/or videos results page 1 of 1

Main filters
Buy Print option
Royalty-Free Option
Reuters Results
Media Type
Orientation
Colour
Rights Type
Rights
More filters
Bridgeman Artists
Bridgeman Photographers
Century
Footage filters
Video Original Format
Video Resolution
Video Category
Filter group
Order By:
per page
Filter group
Rights Type
Media Type
No copyright

Display options

View
Image Size

Images of 'Electromagnetic Spectrum' found, 26

Corby & Browning's mircospectroscope, 1895
Electromagnetic spectrum, neon tube showing a characteristic orange glow.
Content Partner Restrictions
  • Not available to clients invoiced in China
Electromagnetic spectrum, green led, light-emitting diode, showing a green glow .
Content Partner Restrictions
  • Not available to clients invoiced in China
Green, red and blue coloured disks showing the subtractive process, the three filters contain pigments which absorb some of the colours in the white light passing through.
Earth seen by satellite DSCOVR - Earth seen by satellite DSCOVR: Earth photo obtained by satellite Deep Space Climate Observatory (DSCOVR) on July 6, 2015. This satellite, launched on 11 February 2015, and placed in orbit 1.6 million km, at the point of Lagrange L1 (about 4 times farther than the Moon's orbit), provides views of the Earth as a whole - The journey has been a long one for the Deep Space Climate Observatory (DSCOVR). Once known as Triana, the satellite was conceived in 1998 to provide continuous views of Earth, to monitor the solar wind, and to measure fluctuations in Earth's albedo. The mission was put on hold in 2001, and the part-built satellite ended up in storage for several years with an uncertain future. In 2008, the National Oceanic and Atmospheric Administration (NOAA), NASA, and the U.S. Air Force decided to refurbish and update the spacecraft for launch - On February 11, 2015, DSCOVR was finally lofted into space by a SpaceX Falcon 9 rocket. After journey of about 1.6 million kilometers (1 million miles) to the L1 Lagrange Point, the satellite and its Earth Polychromatic Imaging Camera (EPIC) has returned its first view of the entire sunlit side of Earth. At L1-four times farther than the orbit of the Moon - the gravitational pull of the Sun and Earth cancel out, providing a stable orbit and a continuous view of Earth. The image above was made by combining information from Epic's red, green, and blue bands. (Bands are narrow regions of the electromagnetic spectrum to which a remote sensing instrument responds. When EPIC collects data, it takes a series of 10 images at different bands - from ultraviolet to near infrared.)
Hofmann's spectroscope, 1895
Gustav Kirchhoff, German physicist, c 1860s
Content Partner Restrictions
  • Not available to clients invoiced in the UK
Gustav Robert Kirchhoff, German physicist, c 1870s
Content Partner Restrictions
  • Not available to clients invoiced in the UK
Gustav Robert Kirchhoff, German physicist, c 1860s
Content Partner Restrictions
  • Not available to clients invoiced in the UK
Gustav Kirchhoff, German physicist, mid-19th century
Content Partner Restrictions
  • Not available to clients invoiced in the UK
False colour image of a solar flare photographed from Skylab, 1973 Solar flares are sudden outbursts of energy originating on the Sun's surface and projecting far into its atmosphere
Post-flare loop above the Sun's surface, false colour photograph by Skylab, 1973
Content Partner Restrictions
  • Not available to clients invoiced in the UK
Solar flare eruption in extreme ultraviolet light, photographed from Skylab, 1973
Content Partner Restrictions
  • Not available to clients invoiced in the UK
False colour photograph of the Sun and the Moon, taken from Skylab, 1970s
Content Partner Restrictions
  • Not available to clients invoiced in the UK
Large solar flare seen in extreme ultraviolet light, 1973
Content Partner Restrictions
  • Not available to clients invoiced in the UK
Japet, satellite of Saturn, seen by Cassini - Crescent of Iapetus seen by Cassini spacecraft. - Mosaic in fake colors of Japet, a satellite of 1436 kilometers in diameter, taken by the Cassini probe on 10 September 2007 has a distance of 83 000 km from the satellite. Iapetus, 1,468 kilometers (912 miles) across, seen here in false color, is unique in its dramatic variation in brightness between the northern polar region and the middle and low latitudes. Equally prominent is the moon's equatorial ridge of towering mountains. The profile of the ridge against the darkness of space reveals that it is topped by a cratered plateau approximately 15 kilometers (9 miles) wide. Further west, the profile of the ridge changes from a long plateau to discrete peaks. The mosaic consists of four image footprints across the surface of Iapetus and has a resolution of 489 meters (0.3 miles) per pixel. The color seen in this view represents an expansion of the wavelength region of the electromagnetic spectrum visible to human eyes. The intense reddish - brown hue of the dark material is far less pronounced in true color images. The use of enhanced color makes the reddish character of the dark material more visible than it would be to the naked eye. In addition, the scene has been brightened to improve the visibility of surface features. This view was acquired with the Cassini spacecraft narrow - angle camera on Sept. 10, 2007, at a distance of about 83,000 kilometers (51,600 miles) from Iapetus
Solar flare seen in helium 3 light, photographed from Skylab, 1973
Content Partner Restrictions
  • Not available to clients invoiced in the UK
Post-flare loop above the Sun's surface, ultraviolet photograph from Skylab, 1973
Content Partner Restrictions
  • Not available to clients invoiced in the UK
False colour image of the solar corona, photographed from Skylab, 1973
Content Partner Restrictions
  • Not available to clients invoiced in the UK
Solar flare eruption in false colour, photographed from Skylab, 1973
Content Partner Restrictions
  • Not available to clients invoiced in the UK
Barree spiral galaxy NGC 3259 in the Great Bear - Barred spiral galaxy NGC 3259 in Ursa Major - The barree spiral galaxy NGC 3259 is located about 110 million years away - light from Earth. This galaxy houses a black hole in its heart as well as large zones of star formation in its arms. This image was taken by the Hubble Space Telescope (HST). This classic shot of a galaxy in the constellation of Ursa Major was taken by the NASA/ESA Hubble Space Telescope. NGC 3259 is a bright barred spiral galaxy located approximately 110 million light - years from Earth. Being a fully - formed active galaxy, its bright central bulge hosts a supermassive black hole, whose huge appetite for matter explains the high luminosity of the galaxy's core: as it devours its surroundings, the black hole emits intense radiation across the whole electromagnetic spectrum, including in visible light. The beautiful spiral arms of the galaxy are not left out either as they contain dark lanes of dust and gas, ideal spawning grounds for stars. These bright, young, hot stars appear in rich clusters in the galaxy's arms and are what gives the galaxy its blueish hue. Interestingly, the galaxy has a small companion (visible to the left of the image), a much smaller galaxy that may be orbiting NGC 3259. In the background, numerous distant galaxies can be seen, easily identifiable by their elliptical shapes. They are visible here mainly in infrared light, which is shown in red in this image
Crab Nebula seen in different wavelength - The Crab Nebula in multi wavelength: M1, the Crab Nebula, is the rest of a supernova that exploded on July 4, 1054. It is located about 6500 light years from Earth in the constellation Taurus. At the heart of this nebula is a pulsar. To obtain this photo, different observatories and telescopes combined their observations; the VLA provided the radio image (in red), the Spitzer telescope the infrared image (in yellow), the Hubble telescope for the visible part (here in green), XMM-Newton the ultraviolet image (in blue) and the Chandra telescope for X-ray data (purple). The pulsar is the bright spot in the center of the image. The unusual image was produced by combining data from telescopes spanning almost the entire electromagnetic spectrum, from radio waves to X-rays. The Karl G. Jansky Very Large Array (VLA) provided information about the nebula gathered in the radio regime (colored in red). Nasa's Spitzer Space Telescope took images in the infrared (yellow). The NASA/ESA Hubble Space Telescope provided the images made in optical wavelengths (colored in green). ESA's XMM-Newton telescope observed the Crab Nebula in the ultraviolet (blue) and Nasa's Chandra X-ray Observatory provided the data for X-ray radiation (purple). The Crab Nebula, located 6500 light-years from Earth in the constellation of Taurus, is the result of a supernova explosion which was observed by Chinese and other astronomers in 1054. At its centre is a pulsar: a super-dense neutron star, spinning once every 33 milliseconds, shooting out rotating light-like beams of radio waves and visible light. Surrounding the pulsar lies a mix of material; some of it was originally expelled from the star before it went supernova, and the rest was ejected during the explosion itself. Fast-moving winds of particles fly off from the neutron star, energising the dust and gas around it.
Map of the sky seen by Planck - The microwave sky as seen by Planck - 380,000 years after the formation of the universe, when the temperature had become low enough, the light could be released from the extremely dense material that imprisoned it and spread throughout the universe. This moment appears to us today in the form of a radiation called fossil radiation, or cosmological diffuse background. This image is the map of temperature fluctuations of the cosmological diffuse background (in orange) seen by the Planck satellite between August 2009 and June 2010. Overlay, in blue, the Lactee Way and clear, filamentary structures that extend beyond the plane of our Lactee Way. This multi-frequency all-sky image of the microwave sky has been composed using data from Planck covering the electromagnetic spectrum from 30 GHz to 857 GHz. The mottled structure of the CMBR, with its tiny temperature fluctuations reflecting the primordial density variations from which today's cosmic structure originated, is clearly visible in the high-latitude regions of the map. The central band is the plane of our Galaxy. A large portion of the image is dominated by the diffuse emission from its gas and dust. The image was derived from data collected by Planck during its first all-sky survey and comes from observations taken between August 2009 and June 2010. To the right of the main image, below the plane of the Galaxy, is a large cloud of gas in our Galaxy. The obvious arc of light surrounding it is Barnard's Loop - the expanding bubble of an exploded star. Planck has seen whole other galaxies. The great spiral galaxy in Andromeda, 2.2 million light-years from Earth, appears as a sliver of microwave light, released by the coldest dust in its giant body. Other, more distant, galaxies with supermassive black holes appear as single points of microwaves dotting the image
Remains of the supernova Kepler in Ophiuchus - Nasa's three Great Observatories - - the Hubble Space Telescope, the Spitzer Space Telescope, and the Chandra X - ray Observatory - joined forces to probe the expanding remains of a supernova, called Kepler's supernova remnant, first seen 400 years ago by sky watchers, including famous astronomer Johannes Kepler. The combined image unveils a bubble - shaped shroud of gas and dust that is 14 light - years wide and is expanding at 4 million miles per hour (2,000 kilometers per second). Observations from each telescope highlight distinct features of the supernova remnant, a fast - moving shell of iron - rich material from the exploded star, surrounded by an expanding shock wave that is sweeping up interstellar gas and dust. Each color in this image represents a different region of the electromagnetic spectrum, from X - rays to infrared light. The X - ray and infrared data cannot be seen with the human eye. By color - coding those data and combining them with Hubble's visible - light view, astronomers are presenting a more complete picture of the supernova remnant. Visible - light images from the Hubble telescope's Advanced Camera for Surveys [colored yellow] reveal where the supernova shock wave is slamming into the densest regions of surrounding gas. The bright glowing knots are dense clumps from instabilities that form behind the shock wave. The Hubble data also show thin filaments of gas that look like rippled sheets seen edge - on. These filaments reveal where the shock wave is encountering lower - density, more uniform interstellar material. The Spitzer telescope shows microscopic dust particles [colored red] that have been heated by the supernova shock wave. The dust re - radiates the shock wave's energy as infrared light. The Spitzer data are brightest in the regions surrounding those seen in detail by the Hubble telescope. The Chandra X - ray data show regions of very hot gas, and extremely high - energy particles