Results 41 to 50 of about 54,745 (274)

Coronal Mass Ejections over Solar Cycles 23 and 24

Space Science Reviews, 2019
We present a statistical analysis of solar coronal mass ejections (CMEs) based on 23 years of quasi-continuous observations with the LASCO coronagraph, thus covering two complete Solar Cycles (23 and 24).
P. Lamy, O. Floyd, B. Boclet, J. Wojak, H. Gilardy, T. Barlyaeva   +5 more
semanticscholar   +1 more source

A solar storm observed from the Sun to Venus using the STEREO, Venus Express, and MESSENGER spacecraft [PDF]

, 2009
The suite of SECCHI optical imaging instruments on the STEREO-A spacecraft is used to track a solar storm, consisting of several coronal mass ejections (CMEs) and other coronal loops, as it propagates from the Sun into the heliosphere during May 2007 ...
Forsyth, R., Coates AJ, Davies, JA, Thernisien, A, Brown, D., Harrison, R. A., R. J. Forsyth, Lockwood, M., C. J. Davis, Crothers, S., Frahm, R. A., Carr, CM, M. Grande, Bewsher, D, Winningham JD, Savani, NP, Howard, RA, Eyles, C.J., Tsang S, Davis CJ, M. Fränz, N. P. Savani, Howard, R. A., Grande, M, Hapgood, M., Savani NP, Winningham, JD, Crothers SR, Grande, M., Savani, N.P., Harrison RA, Davies, J. A., Bewsher, D., Forsyth, RJ, Davies, J., M. Hapgood, Anderson, B., Sheeley, N.R., Winningham, J., Eyles, C., Tsang, S., Hapgood, M, Fränz M, Whittaker I, C. J. Eyles, G. H. Jones, Davies JA, Grande M, Harrison, R.A., R. A. Frahm, J. D. Winningham, Forsyth, R.J., Whittaker, I., Brown DS, Anderson, B, Zhang, T.-L., S. Tsang, Howard, R., R. A. Howard, Forsyth RJ, M. Lockwood, Sheeley, N. R., Brown, Daniel Stephen, Winningham, J. D., Frahm, R.A., Bewsher D, Savani, N., Rouillard AP, Sheeley NR, Zhang, TL, Coates, AJ, Davis, CJ, Lockwood M, Whittaker, I, Savani, N. P., Frahm, R., I. Whittaker, Eyles, C. J., Jones, G. H., Harrison, R., A. Thernisien, Eyles CJ, Thernisien A, Davis, C., Forsyth, R. J., Frahm, RA, Davis, C.J., Eyles, Christopher, Thernisien, A., T.-L. Zhang, Rouillard, A., Zhang, T., Rouillard, A.P., Bewsher, Danielle, Rouillard, A. P., Zhang, T. -L., Howard RA, Crothers, S.R., Jones, G.H., Fränz, M., Sheeley, N., D. S. Brown, Tsang, S, Rouillard, AP, Davis, C. J., Hapgood M, Brown, D.S., Jones, G., S. R. Crothers, Carr CM, A. J. Coates, Carr, C.M., B. Anderson, Winningham, J.D., Frahm RA, A. P. Rouillard, J. A. Davies, Scott, Chris J., Davies, J.A., Coates, A., C. M. Carr, Carr, C. M., Howard, R.A., Coates, A.J., Harrison, RA, N. R. Sheeley, Fraenz, M., Brown, DS, Brown, D. S., Jones GH, Sheeley, NR, Lockwood, M, Coates, A. J., D. Bewsher, Crothers, S. R., Zhang T, Carr, C., Crothers, SR, Jones, GH, Anderson B, Fränz, M, R. A. Harrison   +141 more
core   +1 more source

Microwave radio emissions as a proxy for coronal mass ejection speed in arrival predictions of interplanetary coronal mass ejections at 1 AU

Journal of Space Weather and Space Climate, 2017
The propagation of a coronal mass ejection (CME) to the Earth takes between about 15 h and several days. We explore whether observations of non-thermal microwave bursts, produced by near-relativistic electons via the gyrosynchrotron process, can be used ...
Matamoros Carolina Salas, Klein Karl Ludwig, Trottet Gerard   +2 more
doaj   +1 more source

Simultaneous interplanetary scintillation and Heliospheric Imager observations of a coronal mass ejection [PDF]

, 2008
We describe simultaneous Interplanetary Scintillation (IPS) and STEREO Heliospheric Imager (HI) observations of a coronal mass ejection (CME) on 16 May 2007. Strong CME signatures were present throughout the IPS observation.
Rouillard AP, Fallows, R. A., Rouillard, Alexis, Dorrian, G. D., Davies, J.A., Dorrian GD, Rouillard, A.P., Brown DS, Rouillard, A. P., Breen, A. R., Brown, D.S., Brown, Daniel, Fallows, R.A., Davies, Jackie, Breen, Andy, Fallows RA, Davies, J. A., Brown, Daniel Stephen, Davies JA, Dorrian, G.D., Fallows, Richard, Breen AR, Breen, A.R., Dorrian, Gareth   +23 more
core   +1 more source

First imaging of corotating interaction regions using the STEREO spacecraft [PDF]

, 2008
Plasma parcels are observed propagating from the Sun out to the large coronal heights monitored by the Heliospheric Imagers (HI) instruments onboard the NASA STEREO spacecraft during September 2007. The source region of these out-flowing parcels is found
Rouillard AP, Davies, JA, Harrison, R. A., Davis, CJ, R. J. Forsyth, Lockwood, M., C. J. Davis, Lockwood M, Rees A, Eyles, C. J., Perry, C.H., Eyles CJ, Forsyth, R. J., Bewsher, D, Davis, C.J., Eyles, Christopher, Eyles, C.J., Davis CJ, Bewsher, Danielle, Rouillard, A. P., A. Rees, Hapgood, M., Crothers SR, Perry, C. H., Crothers, S.R., Rees, A, Harrison RA, Davies, J. A., Bewsher, D., Perry CH, Rouillard, AP, Forsyth, RJ, Davis, C. J., Hapgood M, M. Hapgood, Rouillard, Alexis P., Hapgood, M, S. R. Crothers, C. J. Eyles, Davies JA, Perry, CH, Harrison, R.A., A. P. Rouillard, J. A. Davies, Scott, Chris J., Forsyth, R.J., Davies, J.A., Harrison, RA, Lockwood, Michael, Lockwood, M, D. Bewsher, Crothers, S. R., Crothers, SR, Forsyth RJ, M. Lockwood, Rees, A., R. A. Harrison, Bewsher D, C. H. Perry   +58 more
core   +1 more source

A Comparative Study of Two Contrasting Cosmic-Ray Events Caused by Solar Eruptions from NOAA AR 12673 in 2017 September

The Astrophysical Journal, 2023
Two major solar eruptions on AR 12673 produced a Forbush decrease (FD) event (reduction of cosmic rays) on 2017 September 8 and ground-level enhancement (GLE; enhancement of cosmic rays) on 2017 September 10.
Xiao Xia Yu, Shuang Nan Zhang, Hong Lu, Hong Bo Hu, Ping Zhang, Wei Kang Gao   +5 more
doaj   +1 more source

Editorial to the Special Issue “Propagation of Coronal Mass Ejections”

Universe, 2023
Coronal mass ejections (CMEs) and their associated shocks are one of the main drivers of heliosphere variability, causing both interplanetary and planetary perturbations [...]
Mateja Dumbović, Fang Shen
doaj   +1 more source

Periodicities in solar coronal mass ejections [PDF]

Monthly Notices of the Royal Astronomical Society, 2003
Mid-term quasi-periodicities in solar coronal mass ejections (CMEs) during the most recent solar maximum cycle 23 are reported here for the first time using the four-year data (February 5, 1999 to February 10, 2003) of the Large Angle Spectrometric Coronagraph (LASCO) onboard the Solar and Heliospheric Observatory (SOHO).
Lou, Y. -Q., Wang, Y. -M., Fan, Z., Wang, S., Wang, J.   +4 more
openaire   +2 more sources

Particle precipitation during ICME-driven and CIR-driven geomagnetic storms [PDF]

, 2008
Interplanetary coronal mass ejections (ICME) and corotating interaction regions (CIR) alter the parameters of the solar wind and interplanetary magnetic field (IMF) that affect conditions in the Earth's magnetosphere and particle precipitation in the ...
N. Longden, Honary, Farideh, Denton, Michael H., F. Honary, Longden, N., M. H. Denton   +5 more
core   +1 more source

3D reconstruction of coronal loops by the principal component analysis [PDF]

, 2013
Knowing the three dimensional structure of plasma filaments in the uppermost part of the solar atmosphere, known as coronal loops, and especially their length, is an important parameter in the wave-based diagnostics of this part of the Sun.
Nisticò, Giuseppe, Valery Nakariakov, Giuseppe Nisticò, Erwin Verwichte, Valery M. Nakariakov, Verwichte, E. (Erwin), Nakariakov, V. M. (Valery M.)   +6 more
core   +1 more source