Search Publications

GNSS measurement of EUV photons flux rate during strong and mid solar flares
DOI: 10.1029/2012SW000826 Bibcode: 2012SpWea..1012001H

Hernández-Pajares, M.; García-Rigo, A.; Juan, J. M. +3 more

A new GNSS Solar Flare Activity Indicator (GSFLAI) is presented, given by the gradient of the ionospheric Vertical Total Electron Content (VTEC) rate, in terms of the solar-zenithal angle, measured from a global network of dual-frequency GPS receivers. It is highly correlated with the Extreme Ultraviolet (EUV) photons flux rate at the 26-34 nm spe…

2012 Space Weather
SOHO 32
Wang-Sheeley-Arge-Enlil Cone Model Transitions to Operations
DOI: 10.1029/2011SW000663 Bibcode: 2011SpWea...9.3004P

Odstrcil, Dusan; Pizzo, Vic; Millward, George +3 more

The National Weather Service's (NWS) Space Weather Prediction Center (SWPC) is transitioning the first large-scale, physics-based space weather prediction model into operations on the NWS National Centers for Environmental Prediction (NCEP) supercomputing system (see also C. Schultz, Space weather model moves into prime time, Space Weather, 9, S03…

2011 Space Weather
SOHO 100
A tool for empirical forecasting of major flares, coronal mass ejections, and solar particle events from a proxy of active-region free magnetic energy
DOI: 10.1029/2009SW000537 Bibcode: 2011SpWea...9.4003F

Falconer, David; Barghouty, Abdulnasser F.; Khazanov, Igor +1 more

This paper describes a new forecasting tool developed for and currently being tested by NASA's Space Radiation Analysis Group (SRAG) at Johnson Space Center, which is responsible for the monitoring and forecasting of radiation exposure levels of astronauts. The new software tool is designed for the empirical forecasting of M- and X-class flares, c…

2011 Space Weather
SOHO 80
Geoeffectiveness (Dst and Kp) of interplanetary coronal mass ejections during 1995-2009 and implications for storm forecasting
DOI: 10.1029/2011SW000670 Bibcode: 2011SpWea...9.7005R

Cane, H. V.; Richardson, I. G.

We summarize the geoeffectiveness (based on the Dst and Kp indices) of the more than 300 interplanetary coronal mass ejections (ICMEs) that passed the Earth during 1996-2009, encompassing solar cycle 23. We subsequently estimate the probability that an ICME will generate geomagnetic activity that exceeds certain thresholds of Dst or Kp, including …

2011 Space Weather
SOHO 62
Validation of community models: 3. Tracing field lines in heliospheric models
DOI: 10.1029/2011SW000665 Bibcode: 2011SpWea...910003M

MacNeice, Peter; Elliott, Brian; Acebal, Ariel

Forecasting hazardous gradual solar energetic particle (SEP) bursts at Earth requires accurately modeling field line connections between Earth and the locations of coronal or interplanetary shocks that accelerate the particles. We test the accuracy of field lines reconstructed using four different models of the ambient coronal and inner heliospher…

2011 Space Weather
SOHO 32
A comparison of space weather analysis techniques used to predict the arrival of the Earth-directed CME and its shockwave launched on 8 April 2010
DOI: 10.1029/2010SW000620 Bibcode: 2011SpWea...9.1005D

Webb, D. F.; Möstl, C.; Farrugia, C. J. +10 more

The Earth-directed coronal mass ejection (CME) of 8 April 2010 provided an opportunity for space weather predictions from both established and developmental techniques to be made from near-real time data received from the SOHO and STEREO spacecraft; the STEREO spacecraft provide a unique view of Earth-directed events from outside the Sun-Earth lin…

2011 Space Weather
SOHO 30
Modeling of coronal mass ejections that caused particularly large geomagnetic storms using ENLIL heliosphere cone model
DOI: 10.1029/2010SW000642 Bibcode: 2011SpWea...9.6002T

Odstrcil, D.; Kuznetsova, M.; Hesse, M. +3 more

In our previous paper we reported the results of modeling of 14 selected well-observed strong halo coronal mass ejection (CME) events using the WSA-ENLIL cone model combination. Cone model input parameters were obtained from white light coronagraph images of the CME events using the analytical method developed by Xie et al. (2004). This work verif…

2011 Space Weather
SOHO 23
Evaluating predictions of ICME arrival at Earth and Mars
DOI: 10.1029/2011SW000682 Bibcode: 2011SpWea...9.0E12F

Odstrcil, D.; Vennerstrom, S.; Falkenberg, T. V. +5 more

We present a study of interplanetary coronal mass ejection (ICME) propagation to Earth and Mars. Because of the significant space weather hazard posed by ICMEs, understanding and predicting their arrival and impact at Mars is important for current and future robotic and manned missions to the planet. We compare running ENLILv2.6 with coronal mass …

2011 Space Weather
SOHO 17
Earth-Moon-Mars Radiation Environment Module framework
DOI: 10.1029/2009SW000523 Bibcode: 2010SpWea...8.0E02S

Schwadron, N. A.; Posner, A.; Dayeh, M. A. +11 more

We are preparing to return humans to the Moon and setting the stage for exploration to Mars and beyond. However, it is unclear if long missions outside of low-Earth orbit can be accomplished with acceptable risk. The central objective of a new modeling project, the Earth-Moon-Mars Radiation Exposure Module (EMMREM), is to develop and validate a nu…

2010 Space Weather
Ulysses 66
Validation of SWMF magnetic field and plasma
DOI: 10.1029/2009SW000494 Bibcode: 2010SpWea...8.3002W

Ridley, A. J.; Welling, D. T.

The Space Weather Modeling Framework (SWMF), using the coupled BATSRUS model, the Rice Convection Model, and an ionosphere electrodynamics solver, is used to simulate 10 space weather events. The simulations are completed in near real time using a limited amount of computational resources. Satellite-specific magnetic field, plasma energy-density s…

2010 Space Weather
Cluster 54