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2023-03-TP-01

Start Time: 2023-03-21T00:00:00Z

End Time: 2023-03-28T00:00:00Z

Solar Cycle: 25

Space Weather Impacts:

Comment/Notes:




	

Observed Max Indices :

Index TimeStamp Min/Max Value Source
Quicklook-hourly-Dst 2023-03-24T02:00:00Z -184.0 World Data Center for Geomagnetism, Kyoto (via iSWA HAPI API)
Provisional-hourly-Dst 2023-03-24T02:00:00Z -163.0 World Data Center for Geomagnetism, Kyoto (via iSWA HAPI API)
1-minute SYM/H index 2023-03-24T05:21:00Z -170.0 World Data Center for Geomagnetism, Kyoto (via CDAWEB HAPI API)
1-minute SYM/H index 2023-03-24T05:22:00Z -170.0 World Data Center for Geomagnetism, Kyoto (via CDAWEB HAPI API)
1-minute SYM/H index 2023-03-24T05:23:00Z -170.0 World Data Center for Geomagnetism, Kyoto (via CDAWEB HAPI API)
3-hour-Kp 2023-03-24T06:00:00Z 8.0 GFZ German Research Centre for Geosciences (via iSWA HAPI API)
3-hour-Ap 2023-03-24T06:00:00Z 207.0 GFZ German Research Centre for Geosciences (via iSWA HAPI API)
Daily local noon-time observed (F10.7obs) solar radio flux F10.7 2023-03-25T00:00:00Z 160.3 Dominion Radio Astrophysical Observatory and Natural Resources Canada (via iSWA HAPI API)
Daily International Sunspot Number (SN) 2023-03-27T00:00:00Z 158.0 Royal Observatory of Belgium, Brussels (via iSWA HAPI API)

Useful Links for users who are interested in this TP (e.g. iSWA layouts, DONKI events, etc.):

  • Plots of Observed Indices on ISWA for this TP
  • CCMC-DONKI-Catalog of all events for this TP
  • DONKI M2M Weekly Space Weather Report for March 22, 2023 - March 28, 2023
  • DONKI-2023-03-23T12:00:00-GST-001
  • The March 2023 Storm Narratives (from Yihua)
  • Publications Studying/Related to this Time Period :

  • T.L. Gulyaeva, Interaction of global electron content with the Sun and solar wind during intense geomagnetic storms, Planetary and Space Science, Volume 240, 2024, 105830, ISSN 0032-0633, https://doi.org/10.1016/j.pss.2023.105830.
  • Rajana, S.S.K., Panda, S.K., Jade, S. et al. Impact of two severe geomagnetic storms on the ionosphere over Indian longitude sector during March-April 2023. Astrophys Space Sci 369, 3 (2024). https://doi.org/10.1007/s10509-024-04268-9
  • Strongest solar storm in nearly 6 years slams into Earth catching forecasters by surprise, Space.com
  • Dobrijevic, Daisy (March 25, 2023), Strongest solar storm since 2017 hits Earth but leaves aurora chasers in the dark, Space.com.
  • Kenpankho, Prasert and Chollada Pansong (2023), Ionospheric Disturbances at Low-latitude during Severe Geomagnetic Storm Events.
  • Le, G., Liu, G., Yizengaw, E., Wu, C.‐C., Zheng, Y., Vines, S., & Buzulukova, N.(2024). Responses of field‐aligned currents and equatorial electrojet to sudden decrease of solar wind dynamic pressure during the March 2023 geomagnetic storm. Geophysical Research Letters, 51, e2024GL109427
  • Oyama, S., Vanhamäki, H., Cai, L., Shinbori, A., Hosokawa, K., Sakanoi, T., et al. (2024). Thermospheric wind response to March 2023 storm: Largest wind ever observed with a Fabry‐Perot interferometer in Tromsø, Norway since 2009. Space Weather, 22, e2023SW003728
  • Phillips, Tony, Severe Geomagnetic Storm: March 23-24, 2023, Spaceweather.com. Retrieved on 4/21/2024 from https://spaceweatherarchive.com/2023/03/25/severe-geomagnetic-storm-march-23-24-2023/
  • Phillips, Tony, The 7th X-flare of 2023 — and it’s only March, Spaceweather.com, Retrieved on 4/21/2024 from https://spaceweatherarchive.com/2023/03/
  • Space Weather Services, Bureau of Meteorology, Australian Government, Solar and Geophysical Summary March 2023, www.sws.bom.gov.au
  • Teng, Weilin, Yingna Su, Haisheng Ji, & Qingmin Zhang (2024), Unexpected major geomagnetic storm caused by faint eruption of a solar trans-equatorial flux rope, Nature Communications (2024) 15:9198.
  • List of CCMC GM Runs Series found matching the time period:

  • SWMF-01_2023-03-TP-01_052423_1
  • SWMF-01_2023-03-TP-01_080123_2
  • SWMF-02_2023-03-TP-01_080223_1
  • MAGE-01_2023-03-TP-01_042224_1
  • List of CCMC IT Runs Series found matching the time period:

  • SAMI3-TIEGCM-01_2023-03-TP-01_081823_IT_1
  • SAMI3-HWM-01_2023-03-TP-01_081823_IT_1
  • TIEGCM-Heelis-01_2023-03-TP-01_012624_IT_2
  • WACCMX-Heelis-01_2023-03-TP-01_012624_IT_5
  • WACCMX-Weimer-01_2023-03-TP-01_012624_IT_6
  • TIEGCM-Weimer-01_2023-03-TP-01_012624_IT_1
  • DTM2013-01_2023-03-TP-01_020924_IT_1
  • DTM2020-01_2023-03-TP-01_020924_IT_2
  • JB2008-01_2023-03-TP-01_020924_IT_5
  • IRI2016-01_2023-03-TP-01_030424_IT_1
  • TIEGCM-Weimer-02_2023-03-TP-01_012624_IT_4
  • TIEGCM-Heelis-02_2023-03-TP-01_012624_IT_3
  • GITM-01a_2023-03-TP-01_021424_IT_1
  • GITM-01b_2023-03-TP-01_021424_IT_2
  • CTIPe-01_2023-03-TP-01_111424_IT_1
  • JB2008-01_2023-03-TP-01_111424_IT_1
  • GITM-01_2023-03-TP-01_011125_IT_1
  • WAMIPE-01_2023-03-TP-01_031625_IT_1
  • List of Other CCMC ROR Runs found matching the time period:

  • spase://CCMC/SimulationRun/VERB-3D/2.5/ROR/Yihua_Zheng_012224_IM_4
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