• No results found

[PDF] Top 20 Ground geomagnetic field and GIC response to March 17, 2015, storm

Has 10000 "Ground geomagnetic field and GIC response to March 17, 2015, storm" found on our website. Below are the top 20 most common "Ground geomagnetic field and GIC response to March 17, 2015, storm".

Ground geomagnetic field and GIC response to March 17, 2015, storm

Ground geomagnetic field and GIC response to March 17, 2015, storm

... Day geomagnetic storm on March 17, 2015, has been chosen by the space community for synergetic analysis to build a more comprehensive picture of the storm’s origin and ...This ... See full document

13

The first super geomagnetic storm of solar cycle 24: “The St  Patrick’s day event (17 March 2015)”

The first super geomagnetic storm of solar cycle 24: “The St Patrick’s day event (17 March 2015)”

... 21 March 2015. For these reasons, we concluded that the super-storm on 17 March 2015 was caused by the southward field in both the sheath and in part of MC17 which was ... See full document

12

April 2000 geomagnetic storm: Ionospheric drivers of large geomagnetically induced currents

April 2000 geomagnetic storm: Ionospheric drivers of large geomagnetically induced currents

... large GIC were associated with ...calized GIC at M¨ants¨al¨a cannot be accounted for by sub- storms, but perhaps by some finer structure behavior of the magnetosphere that was directly driven by the solar ... See full document

9

The asymmetric geospace as displayed during the geomagnetic storm on 17 August 2001

The asymmetric geospace as displayed during the geomagnetic storm on 17 August 2001

... the ground mag- netic field, assuming that they correspond to currents oppo- site of the flow (Hall currents), and that 1 nT corresponds to 2 m s −1 ... See full document

20

Ionospheric TEC Response to Geomagnetic Storms Occurred on 15-20 March 2013 and 2015 over the Eastern Africa Region

Ionospheric TEC Response to Geomagnetic Storms Occurred on 15-20 March 2013 and 2015 over the Eastern Africa Region

... TEC response to geomagnetic storm on 24 August 2005 at Indian low latitude stations, Kumar and Singh [10] revealed the enhancement in TECv which showed positive storm ...electric field ... See full document

9

Enhancement and modulation of cosmic noise absorption in the afternoon sector at subauroral location ( L = 5) during the recovery phase of 17 March 2015 geomagnetic storm

Enhancement and modulation of cosmic noise absorption in the afternoon sector at subauroral location ( L = 5) during the recovery phase of 17 March 2015 geomagnetic storm

... Pc2 geomagnetic oscil- lations at the ...during storm and substorm processes and are considered as potential cause of ring current ion loss during strong geomagnetic ...of geomagnetic ... See full document

17

Recent geomagnetic secular variation from Swarm and ground observatories as estimated in the CHAOS 6 geomagnetic field model

Recent geomagnetic secular variation from Swarm and ground observatories as estimated in the CHAOS 6 geomagnetic field model

... 160 ground observa‑ tories as available in March 2016, to update the CHAOS time‑dependent geomagnetic field ...magnetic field between ...the field intensity in 2015 over a ... See full document

18

The 17 March 2015 storm: the associated magnetic flux rope structure and the storm development

The 17 March 2015 storm: the associated magnetic flux rope structure and the storm development

... the 17 March 2015 storm and (2) to gain an insight into how the storm developed responding to the solar wind ...the storm development, we first estimate the injection rate of the ... See full document

11

Enhancement and modulation of cosmic noise absorption in the afternoon sector at subauroral location ( L = 5) during the recovery phase of 17 March 2015 geomagnetic storm

Enhancement and modulation of cosmic noise absorption in the afternoon sector at subauroral location ( L = 5) during the recovery phase of 17 March 2015 geomagnetic storm

... ◦ Hiss generated huge precipitations in afternoon sector at high latitude ◦ Localized concurrent Pc5 oscillations in geomagnetic field and CNA during recovery phase of 17th March 2015 St[r] ... See full document

47

Dependence of the high latitude plasma irregularities on the auroral activity indices: a case study of 17 March 2015 geomagnetic storm

Dependence of the high latitude plasma irregularities on the auroral activity indices: a case study of 17 March 2015 geomagnetic storm

... Day storm of 17 March ...2500 ground-based Global Positioning System (GPS) receivers was used to estimate the irregularities occurrence and dynamics over the auroral region of the Northern ... See full document

12

Characterization of the South Atlantic Anomaly

Characterization of the South Atlantic Anomaly

... horizontal geomagnetic field component measured at the magnetic Equator is caused by the intense current flowing in the equatorial ionosphere (Hamid et ...omagnetic field using the global network of ... See full document

11

New advantages of the combined GPS and GLONASS observations for high latitude ionospheric irregularities monitoring: case study of June 2015 geomagnetic storm

New advantages of the combined GPS and GLONASS observations for high latitude ionospheric irregularities monitoring: case study of June 2015 geomagnetic storm

... a ground- based receiver to a GPS ...the ground-based stations can track both systems simultaneously, ...sparse ground-based stations, particularly, at high latitudes of both hemispheres, the Asian ... See full document

14

Chorus acceleration of radiation belt relativistic electrons during March 2013 geomagnetic storm

Chorus acceleration of radiation belt relativistic electrons during March 2013 geomagnetic storm

... 2–3.6 MeV) or 2 (for 4.5 MeV) orders of magnitude higher than the main phase levels. The flux enhance- ments should come from both nonadiabatic process and Dst effect. However, Dst effect appears to play a less important ... See full document

10

Stochastic forecasting of the geomagnetic field from the COV OBS x1 geomagnetic field model, and candidate models for IGRF 12

Stochastic forecasting of the geomagnetic field from the COV OBS x1 geomagnetic field model, and candidate models for IGRF 12

... al. 2015). The CHAOS- 4 estimate of the crustal field (for degrees 15 to 85) was removed from all data, but no correction was applied for the external field since, in COV-OBS type models, a simple ... See full document

14

Dynamics of a geomagnetic storm on 7–10 September 2015 as observed by TWINS and simulated by CIMI

Dynamics of a geomagnetic storm on 7–10 September 2015 as observed by TWINS and simulated by CIMI

... Spence, H. E., Reeves, G. D., Baker, D. N., Blake, J. B., Bolton, M., Bourdarie, S., Chan, A. A., Claudepherre, S. G., Clemmons, J. H., Cravens, J. P., Elkington, S. R., Fennell, J. F., Friedel, R. H. W., Funsten, H. O., ... See full document

18

Ionospheric response to a geomagnetic storm during November 8–10, 2004

Ionospheric response to a geomagnetic storm during November 8–10, 2004

... SHAR) is greater than 1, it indicates the presence of an anomaly, and if it is less than 1 it indicates the inhibition of an anomaly. The examination of the EIA proxy-SHAR on November 8 (Fig. 3(c)) reveals that the ratio ... See full document

8

Global and local Joule heating during substorms in St  Patrick’s Day 2015 geomagnetic storm

Global and local Joule heating during substorms in St Patrick’s Day 2015 geomagnetic storm

... providing geomagnetic indices such as AL index and Wp index and SuperMAG network (http://super ...parameter. Ground magnetometer data, including IL index, taken from IMAGE network (http://space ... See full document

16

A satellite footprint visualisation tool

A satellite footprint visualisation tool

... For the satellite dynamics the SGP4 and SDP4 models specified by NORAD were implemented, for the magnetic conjunctions the Tsyganenko model (Version 2003) was implemented. These models have several advantages and ... See full document

129

Radiation belt electron acceleration by chorus waves during the 17 March 2013 storm

Radiation belt electron acceleration by chorus waves during the 17 March 2013 storm

... during geomagnetic storms due to a competition between various loss and acceleration processes [Reeves et ...2012 storm and found that local acceleration driven by whistler-mode chorus waves was able to ... See full document

15

Reaction of electric and meteorological states of the near ground atmosphere during a geomagnetic storm on 5 April 2010

Reaction of electric and meteorological states of the near ground atmosphere during a geomagnetic storm on 5 April 2010

... the geomagnetic storm on 29 to 30 October as a result of the solar cosmic ray (SCR) effect, and it decreased during the Forbush decrease of GCRs with the corre- sponding growth of the electric field ... See full document

8

Show all 10000 documents...