Manolis Georgoulis

958 posts

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Manolis Georgoulis

Manolis Georgoulis

@ManolisKG

Heliophysicist, interested in solar magnetism, solar eruptions and space-weather forecasting. Own views expressed.

Laurel, MD, USA Katılım Eylül 2013
276 Takip Edilen668 Takipçiler
Priyansh Jaswal
Priyansh Jaswal@JaswalPriyansh·
I presented our recent work on the super active region 13664, the perpetrator behind the severe geomagnetic storm of 2024 May 10-11. Interacted with a lot of people. Got to learn new things. @AdamF_Astro @ManolisKG
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ARCHIVED - NASA Sun & Space
Parker Solar Probe has phoned home! After passing just 3.8 million miles from the solar surface on Dec. 24 — the closest solar flyby in history — we have received Parker Solar Probe’s beacon tone confirming the spacecraft is safe. go.nasa.gov/4fIKuTe
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AAS Publishing
AAS Publishing@AAS_Publishing·
STOP! Going to #AAS245 in DC? Before you make your travel plans, ask yourself: do you want to learn how to provide excellent peer-review? If yes then join our Peer review training provided by AAS journal editors!! Join us the morning of Sunday, Jan 12!
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Anastasiya VaBo
Anastasiya VaBo@_Anastasiya_B·
Unfortunately, the account of @SWATNetProject has been compromised and thus is not accessible any more by the editors. We could not restore the access which is a big loss for us. But we still want to engage with you, 530 followers, on the X platform!
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Sunrise Solar Observatory
Sunrise Solar Observatory@Sunrise_III·
A helicopter airlifts #Sunrise_III’s hardware components from the landing site to #NormanWells, a small town by the Mackenzie River. Here you can see the box that held the post-focal instrumentation flying away. The main mirror of #Sunrise_III’s #telescope travelled IN the heli.
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Manolis Georgoulis
Manolis Georgoulis@ManolisKG·
An excellent @CosparHQ 45th Scientific Assembly in Busan last week, organized by a very proud LOC led by James Park. Settings in the southern coast of Korea equally amazing. Honored to give a well-attended talk on the future of Heliophysics missions (photo credit: Shangbin Yang).
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Manolis Georgoulis
Manolis Georgoulis@ManolisKG·
@xudong_sun We have seen this record-breaking behavior in other parameters, too. Beff (effective connected magnetic field strength) peaked at 9+ kG in the region when Halloween 2003 regions did not go above 4 - 4.5 kG (Source: @esaspaceweather A-EFFort service).
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Xudong Sun
Xudong Sun@xudong_sun·
Update: the flux emergence rate on 5/10 (3 days after the previous plot) actually reached all-time high. It is now the record holder.
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Xudong Sun
Xudong Sun@xudong_sun·
AR 13664/8 has pretty high flux emergence rate, comparable to that of AR 12673 that created the 2017 Sep flares. Plot updated from Sun & Norton (2017).
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COSPAR
COSPAR@CosparHQ·
Join scientists around the world at #COSPAR2024 to share, learn & discuss every space topic under (and over) the Sun. But also, explore the wonders of Busan, Korea🇰🇷 Join us. Regular registration closes 3 June ☀️✍🏼➡️ cospar2024.org
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Manolis Georgoulis
Manolis Georgoulis@ManolisKG·
Finally, a GOES X5.7 from NOAA AR 13664 in the early morning hours (UT) of May 11. Still way below what this active region can give! As mentioned already, this will be a long weekend geomagnetically.
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Peter T Gallagher
Peter T Gallagher@petertgallagher·
Aurora from north Dublin, Ireland!
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Manolis Georgoulis
Manolis Georgoulis@ManolisKG·
On top of all this excitement with solar flares and eruptions, I should mention how humbled I feel being acceded officially as a Corresponding Member of the International Academy of Astronautics at @EmbryRiddle during the 4th IAA/SSA Conf! Pledge to work to honor this election!
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Manolis Georgoulis
Manolis Georgoulis@ManolisKG·
NOAA AR 13664 is indeed a Carrington-level region. Strong statement, but there's more: while it can easily launch X5+ flares for a couple of days now, it stays at low X-class with a series of CMEs. What is more important to relax - flaring or shedding helicity away? More to see..
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Manolis Georgoulis
Manolis Georgoulis@ManolisKG·
@jen_k_usa Great questions! No, Lij is not a vector; it's a linear segment connecting the centroids of two opposite-polarity magnetic flux partitions. Lij is not a constant, not even L11. It means the connection length between the ad hoc first positive and the ad hoc first negative polarity
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