Thermospheric and geomagnetic responses to interplanetary coronal mass ejections observed by ACE and GRACE: Statistical results. Issue 10 (9th October 2015)

• Record Type: Journal Article
• Authors: Krauss, S.; Temmer, M.; Veronig, A.; Baur, O.; Lammer, H.
• Is Part Of: Journal of geophysical research. Volume 120:Issue 10(2015:Oct.)
• Page Start: 8848
• Page End: 8860
• Publication Date: 2015-10-09
• Subjects: Coronal mass ejections -- Thermospheric density -- Geomagnetic Index -- GRACE -- ACE -- Orbit Decay; Magnetospheric physics -- Periodicals; Space environment -- Periodicals; Cosmic physics -- Periodicals; Planets -- Atmospheres -- Periodicals; Heliosphere (Astrophysics) -- Periodicals; Geophysics -- Periodicals; 523.01
• DOI: 10.1002/2015JA021702
• Languages: English
• ISSNs: 2169-9380

Abstract

Abstract: For the period July 2003 to August 2010, the interplanetary coronal mass ejection (ICME) catalogue maintained by Richardson and Cane lists 106 Earth‐directed events, which have been measured in situ by plasma and field instruments on board the ACE satellite. We present a statistical investigation of the Earth's thermospheric neutral density response by means of accelerometer measurements collected by the Gravity Recovery And Climate Experiment (GRACE) satellites, which are available for 104 ICMEs in the data set, and its relation to various geomagnetic indices and characteristic ICME parameters such as the impact speed ( v max ), southward magnetic field strength ( B z ). The majority of ICMEs causes a distinct density enhancement in the thermosphere, with up to a factor of 8 compared to the preevent level. We find high correlations between ICME B z and thermospheric density enhancements (≈0.9), while the correlation with the ICME impact speed is somewhat smaller (≈0.7). The geomagnetic indices revealing the highest correlations are D s t and SYM‐H (≈0.9); the lowest correlations are obtained for K p and A E (≈0.7), which show a nonlinear relation with the thermospheric density enhancements. Separating the response for the shock‐sheath region and the magnetic structure of the ICME, we find that the Dst and SYM‐H reveal a tighter relation to the B z minimum in the magnetic structure of the ICME, whereas the polar cap indices show higher correlations with the B z minimum in the shock‐sheath region. Since the strength of the B z component—either in the sheath or in the magnetic structure of the ICME—is highly correlated (≈0.9) with the neutral density enhancement, we discuss the possibility of satellite orbital decay estimates based on magnetic field measurements at L1, i.e., before the ICME hits the Earth magnetosphere. These results are expected to further stimulate progress in space weather understanding and applications regarding satellite operations. Key Points: Thermospheric and geomagnetic ICME responses are statistically highly correlated Separate analysis of the response for the shock‐sheath region and the magnetic structure of the CME Possibility of neutral density enhancement estimates based on magnetic field measurements