Year |
Citation |
Score |
2020 |
Torbert RB, Dors I, Argall MR, Genestreti KJ, Burch JL, Farrugia CJ, Forbes TG, Giles BL, Strangeway RJ. A New Method of 3‐D Magnetic Field Reconstruction Geophysical Research Letters. 47. DOI: 10.1029/2019Gl085542 |
0.345 |
|
2018 |
Forbes TG, Seaton DB, Reeves KK. Reconnection in the Post-impulsive Phase of Solar Flares The Astrophysical Journal. 858: 70. DOI: 10.3847/1538-4357/Aabad4 |
0.729 |
|
2018 |
Farrugia CJ, Cohen IJ, Vasquez BJ, Lugaz N, Alm L, Torbert RB, Argall MR, Paulson K, Lavraud B, Gershman DJ, Gratton FT, Matsui H, Rogers A, Forbes TG, Payne D, et al. Effects in the Near‐Magnetopause Magnetosheath Elicited by Large‐Amplitude Alfvénic Fluctuations Terminating in a Field and Flow Discontinuity Journal of Geophysical Research. 123: 8983-9004. DOI: 10.1029/2018Ja025724 |
0.445 |
|
2017 |
Torbert RB, Burch JL, Argall MR, Alm L, Farrugia CJ, Forbes TG, Giles BL, Rager A, Dorelli J, Strangeway RJ, Ergun RE, Wilder FD, Ahmadi N, Lindqvist P, Khotyaintsev Y. Structure and Dissipation Characteristics of an Electron Diffusion Region Observed by MMS During a Rapid, Normal-Incidence Magnetopause Crossing Journal of Geophysical Research: Space Physics. 122: 11,901-11,916. DOI: 10.1002/2017Ja024579 |
0.33 |
|
2015 |
Isenberg PA, Forbes TG, Möbius E. Draping of the Interstellar Magnetic Field over the Heliopause: a Passive Field Model The Astrophysical Journal. 805: 153. DOI: 10.1088/0004-637X/805/2/153 |
0.461 |
|
2015 |
Joshi AD, Forbes TG, Park SH, Cho KS. A trio of confined flares in ar 11087 Astrophysical Journal. 798. DOI: 10.1088/0004-637X/798/2/97 |
0.382 |
|
2014 |
Kliem B, J(林隽) L, Forbes T, Priest E, Torok T. Catastrophe versus instability for the eruption of a toroidal solar magnetic flux rope The Astrophysical Journal. 789: 46. DOI: 10.1088/0004-637X/789/1/46 |
0.469 |
|
2014 |
Baty H, Forbes TG, Priest ER. The formation and stability of Petschek reconnection Physics of Plasmas. 21: 112111. DOI: 10.1063/1.4901918 |
0.35 |
|
2014 |
Longcope DW, Forbes TG. Breakout and Tether-Cutting Eruption Models Are Both Catastrophic (Sometimes) Solar Physics. 289: 2091-2122. DOI: 10.1007/S11207-013-0464-8 |
0.457 |
|
2013 |
Huang Y, Bhattacharjee A, Forbes TG. Magnetic reconnection mediated by hyper-resistive plasmoid instability Physics of Plasmas. 20: 082131. DOI: 10.1063/1.4819715 |
0.37 |
|
2013 |
Forbes TG, Priest ER, Seaton DB, Litvinenko YE. Indeterminacy and instability in Petschek reconnection Physics of Plasmas. 20. DOI: 10.1063/1.4804337 |
0.672 |
|
2013 |
Forbes TG. Solar physics: Flares caught in the act Nature Physics. 9: 456-457. DOI: 10.1038/Nphys2703 |
0.395 |
|
2010 |
Savage SL, McKenzie DE, Reeves KK, Forbes TG, Longcope DW. Reconnection outflows and current sheet observed with Hinode/XRT in the 2008 april 9 "CARTWHEEL CME" flare Astrophysical Journal. 722: 329-342. DOI: 10.1088/0004-637X/722/1/329 |
0.694 |
|
2010 |
Reeves KK, Linker JA, Mikić Z, Forbes TG. Current sheet energetics, flare emissions, and energy partition in a simulated solar eruption Astrophysical Journal. 721: 1547-1558. DOI: 10.1088/0004-637X/721/2/1547 |
0.643 |
|
2009 |
Seaton DB, Forbes TG. An analytical model for reconnection outflow jets including thermal conduction Astrophysical Journal. 701: 348-359. DOI: 10.1088/0004-637X/701/1/348 |
0.668 |
|
2009 |
Titov VS, Forbes TG, Priest ER, Mikić Z, Linker JA. Slip-squashing factors as a measure of three-dimensional magnetic reconnection Astrophysical Journal. 693: 1029-1044. DOI: 10.1088/0004-637X/693/1/1029 |
0.425 |
|
2009 |
Baty H, Priest ER, Forbes TG. Petschek-like reconnection with uniform resistivity Physics of Plasmas. 16: 60701. DOI: 10.1063/1.3155087 |
0.402 |
|
2009 |
Baty H, Forbes TG, Priest ER. Petschek reconnection with a nonlocalized resistivity Physics of Plasmas. 16: 12102. DOI: 10.1063/1.3062833 |
0.407 |
|
2008 |
Reeves KK, Seaton DB, Forbes TG. Field line shrinkage in flares observed by the X-ray Telescope on Hinode Astrophysical Journal. 675: 868-874. DOI: 10.1086/526336 |
0.718 |
|
2007 |
Isenberg PA, Forbes TG. A Three-dimensional Line-tied Magnetic Field Model for Solar Eruptions The Astrophysical Journal. 670: 1453-1466. DOI: 10.1086/522025 |
0.504 |
|
2007 |
Reeves KK, Warren HP, Forbes TG. Theoretical predictions of X-ray and extreme-uv flare emissions using a loss-of-equilibrium model of solar eruptions Astrophysical Journal. 668: 1210-1220. DOI: 10.1086/521291 |
0.695 |
|
2007 |
Lin J, Li J, Forbes TG, Ko Y-, Raymond JC, Vourlidas A. Features and properties of coronal mass ejection/flare current sheets The Astrophysical Journal. 658. DOI: 10.1086/515568 |
0.421 |
|
2006 |
Birn J, Forbes TG, Hesse M. Stability and Dynamic Evolution of Three-dimensional Flux Ropes The Astrophysical Journal. 645: 732-741. DOI: 10.1086/504280 |
0.457 |
|
2006 |
Baty H, Priest ER, Forbes TG. Effect of nonuniform resistivity in Petschek reconnection Physics of Plasmas. 13: 22312. DOI: 10.1063/1.2172543 |
0.377 |
|
2006 |
Pick M, Forbes TG, Mann G, Cane HV, Chen J, Ciaravella A, Cremades H, Howard RA, Hudson HS, Klassen A, Klein KL, Lee MA, Linker JA, Maia D, Mikic Z, et al. Multi-wavelength observations of CMEs and associated phenomena: Report of working group F Space Science Reviews. 123: 341-382. DOI: 10.1007/S11214-006-9021-1 |
0.42 |
|
2006 |
Forbes TG, Linker JA, Chen J, Cid C, Kóta J, Lee MA, Mann G, Mikić Z, Potgieter MS, Schmidt JM, Siscoe GL, Vainio R, Antiochos SK, Riley P. CME theory and models: Report of working group D Space Science Reviews. 123: 251-302. DOI: 10.1007/S11214-006-9019-8 |
0.425 |
|
2006 |
Forbes TG, Linker JA, Chen J, Cid C, Kota J, Lee MA, Mann G, Mikic Z, Potgieter MS, Schmidt JM, Siscoe GL, Vainio R, Antiochos SK, Riley P. CME theory and models : Report of working group D Space Science Reviews. 123: 251-302. DOI: 10.1007/978-0-387-45088-9_12 |
0.427 |
|
2005 |
Hesse M, Forbes TG, Birn J. On the Relation between Reconnected Magnetic Flux and Parallel Electric Fields in the Solar Corona The Astrophysical Journal. 631: 1227-1238. DOI: 10.1086/432677 |
0.452 |
|
2005 |
Reeves KK, Forbes TG. Predicted light curves for a model of solar eruptions Astrophysical Journal. 630: 1133-1147. DOI: 10.1086/432047 |
0.69 |
|
2004 |
Sokolov IV, Roussev II, Gombosi TI, Lee MA, Kóta J, Forbes TG, Manchester WB, Sakai JI. A new field line advection model for solar particle acceleration Astrophysical Journal. 616: L171-L174. DOI: 10.1086/426812 |
0.411 |
|
2004 |
Roussev II, Sokolov IV, Forbes TG, Gombosi TI, Lee MA, Sakai JI. A numerical model of a coronal mass ejection: Shock development with implications for the acceleration of GeV protons Astrophysical Journal. 605: L73-L76. DOI: 10.1086/392504 |
0.494 |
|
2004 |
Emslie AG, Kucharek H, Dennis BR, Gopalswamy N, Holman GD, Share GH, Vourlidas A, Forbes TG, Gallagher PT, Mason GM, Metcalf TR, Mewaldt RA, Murphy RJ, Schwartz RA, Zurbuchen TH. Energy partition in two solar flare/CME events Journal of Geophysical Research: Space Physics. 109. DOI: 10.1029/2004Ja010571 |
0.446 |
|
2003 |
Roussev II, Forbes TG, Gombosi TI, Sokolov IV, DeZeeuw DL, Birn J. A three-dimensional flux rope model for coronal mass ejections based on a loss of equilibrium Astrophysical Journal. 588: L45-L48. DOI: 10.1086/375442 |
0.416 |
|
2003 |
Birn J, Forbes TG, Schindler K. Models of Three-dimensional Flux Ropes The Astrophysical Journal. 588: 578-585. DOI: 10.1086/373921 |
0.436 |
|
2003 |
Webb DF, Burkepile J, Forbes TG, Riley P. Observational evidence of new current sheets trailing coronal mass ejections Journal of Geophysical Research. 108: 1440. DOI: 10.1029/2003Ja009923 |
0.517 |
|
2002 |
Lin J, Van Ballegooijen AA, Forbes TG. Evolution of a semicircular flux rope with two ends anchored in the photosphere Journal of Geophysical Research: Space Physics. 107. DOI: 10.1029/2002Ja009486 |
0.485 |
|
2002 |
Priest ER, Forbes TG. The magnetic nature of solar flares The Astronomy and Astrophysics Review. 10: 313-377. DOI: 10.1007/S001590100013 |
0.442 |
|
2001 |
Lin J, Forbes TG, Isenberg PA. Prominence eruptions and coronal mass ejections triggered by newly emerging flux Journal of Geophysical Research. 106: 25053-25073. DOI: 10.1029/2001Ja000046 |
0.447 |
|
2000 |
Birn J, Gosling JT, Hesse M, Forbes TG, Priest ER. Simulations Of Three-Dimensional Reconnection In The Solar Corona The Astrophysical Journal. 541: 1078-1095. DOI: 10.1086/309452 |
0.46 |
|
2000 |
Forbes TG, Lin J. What can we learn about reconnection from coronal mass ejections Journal of Atmospheric and Solar-Terrestrial Physics. 62: 1499-1507. DOI: 10.1016/S1364-6826(00)00083-3 |
0.457 |
|
1999 |
Warren HP, Bookbinder JA, Forbes TG, Golub L, Hudson HS, Reeves K, Warshall A. TRACE and Yohkoh Observations of High-Temperature Plasma in a Two-Ribbon Limb Flare. The Astrophysical Journal. 527: L121-L124. PMID 10577954 DOI: 10.1086/312410 |
0.391 |
|
1998 |
J(林隽) L, Forbes T, Isenberg P, Demoulin P. The Effect of Curvature on Flux-Rope Models of Coronal Mass Ejections The Astrophysical Journal. 504: 1006-1019. DOI: 10.1086/306108 |
0.486 |
|
1996 |
Litvinenko YE, Forbes TG, Priest ER. A strong limitation on the rapidity of flux-pile-up reconnection Solar Physics. 167: 445-448. DOI: 10.1007/Bf00146353 |
0.401 |
|
1995 |
Forbes TG, Priest ER. Photospheric Magnetic Field Evolution and Eruptive Flares The Astrophysical Journal. 446: 377. DOI: 10.1086/175797 |
0.411 |
|
1995 |
Lin J, Forbes TG, Priest ER, Bungey TN. Models for the motions of flare loops and ribbons Solar Physics. 159: 275-299. DOI: 10.1007/Bf00686534 |
0.471 |
|
1993 |
Isenberg PA, Forbes TG, Demoulin P. Catastrophic Evolution of a Force-free Flux Rope: A Model for Eruptive Flares The Astrophysical Journal. 417: 368-386. DOI: 10.1086/173319 |
0.501 |
|
1992 |
Demoulin P, Forbes TG. Weighted current sheets supported in normal and inverse configurations - A model for prominence observations The Astrophysical Journal. 387: 394-402. DOI: 10.1086/171091 |
0.428 |
|
1992 |
Priest ER, Forbes TG. Does fast magnetic reconnection exist Journal of Geophysical Research. 97: 16757-16772. DOI: 10.1029/92Ja01146 |
0.42 |
|
1992 |
Priest ER, Forbes TG. Magnetic flipping: Reconnection in three dimensions without null points Journal of Geophysical Research. 97: 1521-1531. DOI: 10.1029/91Ja02435 |
0.44 |
|
1992 |
Xu P, Forbes TG. The structure of radiative slow-mode shocks Solar Physics. 139: 315-342. DOI: 10.1007/Bf00159157 |
0.463 |
|
1990 |
Schmieder B, Malherbe JM, Simnett GM, Forbes TG, Tandberg-Hanssen E. Evaporation in the Transition Region during the Gradual Phase of Flares The Astrophysical Journal. 356: 720-732. DOI: 10.1086/168879 |
0.408 |
|
1990 |
Priest ER, Forbes TG. The evolution of coronal magnetic fields Solar Physics. 130: 399-402. DOI: 10.1007/Bf00156802 |
0.428 |
|
1989 |
Forbes TG, Malherbe JM, Priest ER. The formation of flare loops by magnetic reconnection and chromospheric ablation Solar Physics. 120: 285-307. DOI: 10.1007/Bf00159881 |
0.477 |
|
1988 |
Forbes TG. Shocks produced by impulsively driven reconnection Solar Physics. 117: 97-121. DOI: 10.1007/Bf00148576 |
0.334 |
|
1987 |
Forbes TG, Priest ER. A comparison of analytical and numerical models for steadily driven magnetic reconnection Reviews of Geophysics. 25: 1583-1607. DOI: 10.1029/Rg025I008P01583 |
0.311 |
|
1986 |
Priest ER, Forbes TG. New models for fast steady state magnetic reconnection Journal of Geophysical Research. 91: 5579-5588. DOI: 10.1029/Ja091Ia05P05579 |
0.406 |
|
1984 |
Forbes TG, Priest ER. Numerical simulation of reconnection in an emerging magnetic flux region Solar Physics. 94: 315-340. DOI: 10.1007/Bf00151321 |
0.498 |
|
1983 |
Forbes TG, Priest ER. On reconnection and plasmoids in the geomagnetic tail Journal of Geophysical Research. 88: 863-870. DOI: 10.1029/Ja088Ia02P00863 |
0.476 |
|
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