Top Tweets for #EOVSA
Coincidentally, today's new study in @ScienceMagazine on predicting large solar flares by Kusano+ looked at the same region that popped the flare we reported in our @NatureAstronomy paper https://t.co/DsbUFwYocC. See story in @AstronomyMag. @NJIT #EOVSA
https://t.co/el9WG24EIm
We are delighted to share that our new @NatureAstronomy paper https://t.co/8SVXH0cXP1, based on observations from #EOVSA & #NASA spacecraft & numerical simulations, is featured by @NSF on its front page. @NJIT @CSLANJIT @CenterForAstro #NSFfunded https://t.co/UW4i4K7Vi6
A short blog post I wrote on the story behind our paper (https://t.co/DsbUFxfZ4a). Particularly I'd like to share the excitement among the @EOVSANJIT team when #EOVSA first captured this spectacular solar flare soon after the instrument was commissioned. @NJIT @CSLANJIT
.@BinChenNJIT delves 'behind the paper' to bring us some insight into the work behind Bin's Nature Astronomy paper, published yesterday: https://t.co/KsZLzSwaC7
#EOVSA observed in microwaves the same flare reported today by the Solar Orbiter X-ray Spectrometer/Telescope (STIX) team. The microwaves show the presence of high energy electrons. Compare the time profiles! #SolarOrbiter #TheSunUpClose @stix_so
#EOVSA can be used to image quiet-Sun features. Images taken on 2020 June 23 show a filament channel, which exhibits in microwave wavelengths as a dark feature due to free-free absorption. Traces of the same filament channel can be seen in H𝛼 and extreme ultraviolet images.
Prof. Dale Gary showing full-disk microwave images from #EOVSA during his talk at the (virtual) #RHESSI Workshop. @EOVSANJIT @CSLANJIT
Now on to the RHESSI workshop ... next talk by Dale Gary from @NJIT showing some spectacular observations from the EOVSA radio telescope ... around the scientific world we go ...
#EOVSA is now on twitter! Our observations in microwaves show a clear, dark filament channel that has traces in H alpha and SDO/AIA 304 angstrom images (sensitive to chromospheric temperature material).
#EOVSA can be used to image quiet-Sun features. Images taken on 2020 June 23 show a filament channel, which exhibits in microwave wavelengths as a dark feature due to free-free absorption. Traces of the same filament channel can be seen in H𝛼 and extreme ultraviolet images.
#EOVSA can be used to image quiet-Sun features. Images taken on 2020 June 23 show a filament channel, which exhibits in microwave wavelengths as a dark feature due to free-free absorption. Traces of the same filament channel can be seen in H𝛼 and extreme ultraviolet images.
Congratulations, #SDO, for one decade of extremely successful operations! And thanks @markcheung for your shoutout to #NJIT’s solar telescopes #EOVSA and #GST! Excited to work with all the wonderful space-borne and grounds-based facilities in the new solar cycle 🙌
In a new paper accepted by ApJL, we used #EOVSA to image microwave emission by nonthermal electrons that follow the erupting magnetic flux rope from the central cavity to its conjugate footprints. Cartoon adapted from @MihoJnvr's 3D standard flare model. https://t.co/JncOLMJr0q
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