High resolution extreme
ultraviolet images from TRACE allowed the solar moss to be observed for the first time, and the rapid cadence with which TRACE takes pictures provided unprecedented details about its behavior.
Ultraviolet images from the Hubble Space Telescope reveal star birth in galaxies that existed 5 billion to 10 billion years ago.
A TANGLED SKEIN Splendid loops in the corona protrude from the sun's surface, seen in this 2014
ultraviolet image from NASA's Solar Dynamics Observatory.
RISE UP Coils of magnetism that erupt from the sun, seen in this false color
ultraviolet image from NASA's Solar Dynamics Observatory, are pushed up in parcels of gas, a new study suggests.
In this extreme
ultraviolet image from NASA's Solar...
Not exact matches
This artist's impression superimposes real visible
images of Jupiter and Europa with
ultraviolet data
from the Hubble Space Telescope showing the plumes (blue).
Images were obtained
from viewing the galaxy in near -
ultraviolet, visible, and near - infrared wavelengths, using the Advanced Camera for Surveys and the Wide Field Camera 3 aboard Hubble.
By utilizing a full spectrum of colour
from ultraviolet to near infared, NASA astronomers have created the most colourful deep space
images to date.
Images from Cassini's
ultraviolet imaging spectrometer (UVIS), obtained
from an unusually close range of about six Saturn radii, provided a look at the changing patterns of faint emissions on scales of a few hundred miles (kilometers) and tied the changes in the auroras to the fluctuating wind of charged particles blowing off the sun and flowing past Saturn.
Ultraviolet and infrared
images from NASA's Cassini spacecraft and Hubble Space Telescope show active and quiet auroras at Saturn's north and south poles.
This
image combines data
from five different telescopes: The VLA (radio) in red; Spitzer Space Telescope (infrared) in yellow; Hubble Space Telescope (visible) in green; XMM - Newton (
ultraviolet) in blue; and Chandra X-ray Observatory (X-ray) in purple.
EPIC takes a series of 10
images using different narrowband spectral filters —
from ultraviolet to near infrared — to produce a variety of science products.
The first
images from the Solar
Ultraviolet Imager or SUVI instrument aboard NOAA's GOES - 16 satellite have been successful, capturing a large coronal hole on Jan. 29, 2017.
Ultraviolet images taken by the Cassini spacecraft revealed the patch, which is distinct
from the planet's auroras.
New Hubble telescope
images show
ultraviolet radiation
from stars born during the universe's adolescent phase.
From the inside out, the «Cassini division» in faint red at left is followed by the A ring in its entirety in this
ultraviolet - light
image.
This sequence of
images of the the Sun in
ultraviolet light was taken by the Solar and Heliospheric Observatory (SOHO) spacecraft on Feb. 11, 1996
from its unique vantage point at the «L1» gravity neutral point 1 million miles sunward
from the Earth.
This
image of the Mars night side shows
ultraviolet emission
from nitric oxide (abbreviated NO).
They are illuminated and heated by a torrent of energetic
ultraviolet light
from its four hottest and most massive stars, called the Trapezium, which lie near the center of the
image.
The WFC3 can capture
images using light across a wide spectrum,
from infrared to
ultraviolet.
Images from the Extreme
ultraviolet Imaging Telescope (EIT) and the Coronal Diagnostics Spectrometer (CDS) on SOHO show the hot gases of the ever - changing corona reacting to the evolving magnetic fields rooted in the solar surface.
Then, they combined the spectra with infrared
images of the Spitzer Space Telescope, the Herschel Space Observatory, and optical
images of the Hubble Space Telescope, to create a complete multi-wavelength picture of their galaxies:
from rest - frame
ultraviolet to rest - frame far - infrared.
Hot stars burn brightly in this
image from NASA's Galaxy Evolution Explorer, showing the
ultraviolet side of a familiar face.
Comparison between the zonal winds
from ultraviolet images and the vertical profile of zonal winds
from the Cassini Composite Infrared Spectrometer (CIRS) shows that the zonal winds
from the
ultraviolet images are
from a pressure level that is ∼ 0.2 scale heights higher than the pressure level of the zonal winds
from continuum - band
images.