Added 04/18/2014 @ 13:20 UTCM7.3
Solar Flare Observed A moderately strong solar flare measuring M7.3 was observed around region 2036 on Friday morning peaking at 13:03 UTC.
Drawing by Valderrama of
the solar flare he observed on 10 September 1886 on a sunspot (with the penumbra shown with hashed lines and the umbra in black).
Solar flare observed by the Reuven Ramaty High Energy Solar Spectroscopic Imager and associated coronal mass ejection observed by the Solar and Heliospheric Observatory spacecraft.
Not exact matches
He conveniently neglects to point out that the seasonal variation
observed was less than 0.1 %, and that the measure variation linked to
solar flares was less than 0.5 %.
More exciting news from the heavens — a major
solar flare that set off Thursday will give metro New York and other areas a very good chance to
observe the aurora borealis (Northern Lights) Saturday evening.
But
solar flares — the brief, intense flashes of light caused by the sun's magnetic fields changing shape suddenly — couldn't be causing the heating because none were
observed.
Trying to
observe the details of Saturn's auroras has essentially been a hit - and - miss proposal, the researchers say: The times at which
solar flares strike the planet aren't readily predictable, and until now the Hubble telescope hasn't been looking at Saturn at the proper wavelengths just when a
solar flare arrived.
How do you figure out what powers
solar flares — the intense bursts of radiation coming from the release of magnetic energy associated with sunspots — when you must rely on
observing only the light and particles that make their way to near - Earth's orbit?
Astronomers at the Harvard - Smithsonian Center for Astrophysics in Cambridge, Massachusetts, studied 84 sunlike stars and
observed 29 of these supersized
solar flares over a 4 - year period to find out how often they occur.
The IRIS team will use information from other satellites that
observe the whole sun, such as Japan's Hinode and NASA's
Solar Dynamics Observatory, to identify active areas of the sun and point IRIS toward
flares as they grow, when it will obtain spectra every two seconds.
At the same time, the Ramaty High - Energy
Solar Spectroscopic Imager (RHESSI) satellite
observed x-rays from a moderate
flare at the same location.
Not long after this, in 1859, Richard Carrington
observed a huge
solar flare that was followed within a day by brilliant displays of the northern lights in regions as far south as Italy and Cuba.
«Furthermore, the white - light
flare observed by Valderrama is, chronologically, the third one recorded in the history of
solar physics,» adds Vaquero.
During the last two months, several of these powerful
solar flares have been
observed, some with associated coronal mass ejections that, in turn, can produce geomagnetic storms that perturb the communication systems in some regions of Earth, especially radio broadcasts and GPS systems.
Scientists studying
solar flares employ special satellites and instruments that do not operate with visible light, but a white - light
flare can be
observed with «normal» telescopes that use visible light, as Valderrama y Aguilar did in 1886.
The successful candidate will work on the analysis and interpretation of
solar flare related radio - bursts
observed with the VLA, in collaboration with our project partner at the New Jersey Institute of Technology, NJ, with the possibility of getting involved in STIX science and operations planning.
Solar prominences (
flares) as
observed by NASA's STEREO mission.
As well as keeping an eye out for
solar flares, it will also be looking well past the Sun to gain a better grasp of the earliest, most distant galaxies we have ever
observed to give astronomers a better idea of what happened in the very early days of our Universe, and perhaps shed light on how the relationship between gravity and dark matter evolved.
Here we present a joint hydrodynamic and radiative model showing that during the first seconds of beam injection the effects caused by beam electrons can reproduce Hα line profiles with large red - shifts closely matching those
observed in a C1.5
flare by the Swedish
Solar Telescope.
«It's very unusual to
observe the opening minutes of a
flare's life,» says Chris Nelson, of Sheffield University's
Solar Physics and Space Plasma Research Centre.
On April 25, 2008, EV Lacertae emitted the brightest
flare by a main - sequence star
observed in the
Solar neighborhood up to that date (more).
This spacecraft was designed to
observe gamma rays, X-rays and UV radiation from
solar flares during a time of high
solar activity.
Solar flares were first
observed by in 1859 by Lord Richard C. Carrington.
British astronomer Richard Carrington noted the coincidence (but did not claim a direct connection) between the auroras and a
solar flare he had
observed the day before, thus prefiguring the discipline of space weather research.
In addition,
solar spectral irradiance instruments aboard TIMED and SORCE have
observed hundreds of
flare events in the 0.1 nm to 190 nm range.