-
1
-
-
0000827017
-
Magnetic fields and the structure of the solar corona
-
Altschuler, M. D., and G. Newkirk Jr. (1969), Magnetic fields and the structure of the solar corona, Sol. Phys., 9, 131-149.
-
(1969)
Sol. Phys
, vol.9
, pp. 131-149
-
-
Altschuler, M.D.1
Newkirk Jr., G.2
-
2
-
-
39449129225
-
J. Geophys. Res., 105
-
A5, 10,465-10, 480
-
Arge, C. N., and V. J. Pizzo (2000), Improvement in the prediction of solar wind conditions using near-real time solar magnetic field updates, J. Geophys. Res., 105(A5), 10,465-10, 480.
-
(2000)
-
-
Arge, C.N.1
Pizzo, V.J.2
-
3
-
-
33751072625
-
Geoeffective analysis of CMEs under current sheet magnetic coordinates
-
doi: 10.1007/s10509-006-9039-6
-
Feng, X. S., and X. H. Zhao (2006), Geoeffective analysis of CMEs under current sheet magnetic coordinates, Astrophys. Space Sci., 111, A09108, doi: 10.1007/s10509-006-9039-6.
-
(2006)
Astrophys. Space Sci
, vol.111
-
-
Feng, X.S.1
Zhao, X.H.2
-
4
-
-
33646559251
-
Modeling the resistive MHD by the CESE method
-
Feng, X. S., Y. Q. Hu, and F. S. Wei (2006), Modeling the resistive MHD by the CESE method, Sol. Phys., 235, 235-257.
-
(2006)
Sol. Phys
, vol.235
, pp. 235-257
-
-
Feng, X.S.1
Hu, Y.Q.2
Wei, F.S.3
-
5
-
-
33847239859
-
A novel numerical implementation for solar wind modeling by the modified conservation element/ solution element method
-
Feng, X. S., Y. F. Zhou, and S. T. Wu (2007), A novel numerical implementation for solar wind modeling by the modified conservation element/ solution element method, Astrophys. J., 655, 1110-1126.
-
(2007)
Astrophys. J
, vol.655
, pp. 1110-1126
-
-
Feng, X.S.1
Zhou, Y.F.2
Wu, S.T.3
-
6
-
-
0031359664
-
Ulysses observations of the northward extension of the heliospheric current sheet
-
Forsyth, R. J., A. Balogh, E. J. Smith, and J. T. Gosling (1997), Ulysses observations of the northward extension of the heliospheric current sheet, Geophys. Res. Lett., 24(20), 3101-3104.
-
(1997)
Geophys. Res. Lett
, vol.24
, Issue.20
, pp. 3101-3104
-
-
Forsyth, R.J.1
Balogh, A.2
Smith, E.J.3
Gosling, J.T.4
-
7
-
-
0042119602
-
North-south asymmetry in the heliospheric current sheet and the IMF sector structure
-
Girish, T. E., and S. R. Prabhakaran Nayar (1988), North-south asymmetry in the heliospheric current sheet and the IMF sector structure, Sol. Phys., 116, 369-376.
-
(1988)
Sol. Phys
, vol.116
, pp. 369-376
-
-
Girish, T.E.1
Prabhakaran Nayar, S.R.2
-
8
-
-
39449135110
-
Global three-dimensional MHD simulation of a space weather event: CME formation, interplanetary propagation, and interaction with the magnetosphere
-
Groth, C. P. T., D. L. D. Zeeuw, T. I. Gombosi, and K. G. Powell (2000), Global three-dimensional MHD simulation of a space weather event: CME formation, interplanetary propagation, and interaction with the magnetosphere, J. Geophys. Res., 105(A11), 25,053-25,078.
-
(2000)
J. Geophys. Res
, vol.105
, Issue.A11
-
-
Groth, C.P.T.1
Zeeuw, D.L.D.2
Gombosi, T.I.3
Powell, K.G.4
-
9
-
-
84905334405
-
-
Hoeksema, J. T., J. M. Wilcox, and P. H. Scherrer (1982), Structure of the heliospheric current sheet in the early portion of sunspot cycle 21, J. Geophys. Res., 87, 10,331-10,338.
-
Hoeksema, J. T., J. M. Wilcox, and P. H. Scherrer (1982), Structure of the heliospheric current sheet in the early portion of sunspot cycle 21, J. Geophys. Res., 87, 10,331-10,338.
-
-
-
-
10
-
-
0020943646
-
-
Hoeksema, J. T., J. M. Wilcox, and P. H. Scherrer (1983), The structure of the heliospheric current sheet: 1978-1982, J. Geophys. Res., 88(A12), 9910-9918.
-
Hoeksema, J. T., J. M. Wilcox, and P. H. Scherrer (1983), The structure of the heliospheric current sheet: 1978-1982, J. Geophys. Res., 88(A12), 9910-9918.
-
-
-
-
11
-
-
0001676717
-
Magnetohydrodynamic modeling of the solar corona during whole Sun month
-
Linker, J. A., Z. Mikić, D. A. Bisecker, R. J. Forsyth, S. E. Gibson, A. J. Lazarus, A. Lecinski, P. Riley, A. Szabo, and B. J. Thompson (1999), Magnetohydrodynamic modeling of the solar corona during whole Sun month, J. Geophys. Res., 104(A5), 9809-9830.
-
(1999)
J. Geophys. Res
, vol.104
, Issue.A5
, pp. 9809-9830
-
-
Linker, J.A.1
Mikić, Z.2
Bisecker, D.A.3
Forsyth, R.J.4
Gibson, S.E.5
Lazarus, A.J.6
Lecinski, A.7
Riley, P.8
Szabo, A.9
Thompson, B.J.10
-
12
-
-
0035217796
-
Including the transition region in models of the large-scale solar corona
-
Lionello, R., J. A. Linker, and Z. Mikić (2001), Including the transition region in models of the large-scale solar corona, Astrophys. J., 546, 542-551.
-
(2001)
Astrophys. J
, vol.546
, pp. 542-551
-
-
Lionello, R.1
Linker, J.A.2
Mikić, Z.3
-
13
-
-
42549104985
-
Solar cycle changes in coronal holes and space weather cycles
-
doi:10.1029/2001JA007550
-
Luhmann, J. G., Y. Li, C. N. Arge, P. R. Gazis, and R. Ulrich (2002), Solar cycle changes in coronal holes and space weather cycles, J. Geophys. Res., 107(A8), 1154, doi:10.1029/2001JA007550.
-
(2002)
J. Geophys. Res
, vol.107
, Issue.A8
, pp. 1154
-
-
Luhmann, J.G.1
Li, Y.2
Arge, C.N.3
Gazis, P.R.4
Ulrich, R.5
-
14
-
-
0013233748
-
Magnetohydrodynamic modeling of the global solar corona
-
Mikić, Z., J. A. Linker, D. D. Schnack, R. Lionello, and A. Tarditi (1999), Magnetohydrodynamic modeling of the global solar corona, Phys. Plasmas, 6(5), 2217-2224.
-
(1999)
Phys. Plasmas
, vol.6
, Issue.5
, pp. 2217-2224
-
-
Mikić, Z.1
Linker, J.A.2
Schnack, D.D.3
Lionello, R.4
Tarditi, A.5
-
15
-
-
19844377633
-
Spatial structure of the solar wind and comparisons with solar data and models
-
Neugebauer, M., et al. (1998), Spatial structure of the solar wind and comparisons with solar data and models, J. Geophys. Res., 103(A7), 14,587-14,599.
-
(1998)
J. Geophys. Res
, vol.103
, Issue.A7
-
-
Neugebauer, M.1
-
17
-
-
0003731716
-
An approximate Riemann solver for magnetohydro-dynamics (that works in more than one dimension),
-
Tech. Rep. 94-24, Inst. for Comput. Appl. in Sci. and Eng, NASA Langley space Flight Center, Hampton, Va
-
Powell, K. G. (1994), An approximate Riemann solver for magnetohydro-dynamics (that works in more than one dimension), Tech. Rep. 94-24, Inst. for Comput. Appl. in Sci. and Eng., NASA Langley space Flight Center, Hampton, Va.
-
(1994)
-
-
Powell, K.G.1
-
18
-
-
33846399995
-
A comparison between global solar magnetohydrody- namic and potential field source surface model results
-
Riley, P., J. A. Linker, Z. Mikić, R. Lionello, S. A. Ledvina, and J. G. Luhmann (2006), A comparison between global solar magnetohydrody- namic and potential field source surface model results, Astrophys. J., 653, 1510-1516.
-
(2006)
Astrophys. J
, vol.653
, pp. 1510-1516
-
-
Riley, P.1
Linker, J.A.2
Mikić, Z.3
Lionello, R.4
Ledvina, S.A.5
Luhmann, J.G.6
-
19
-
-
1142297869
-
Observation of the Sun's magnetic field during the recent solar maximum
-
doi:10.1029/2002JA009388
-
Sanderson, T. R., T. Tappourchaux, J. T. Hoeksema, and K. L. Harvey (2003), Observation of the Sun's magnetic field during the recent solar maximum, J. Geophys. Res., 108(A1), 1035, doi:10.1029/2002JA009388.
-
(2003)
J. Geophys. Res
, vol.108
, Issue.A1
, pp. 1035
-
-
Sanderson, T.R.1
Tappourchaux, T.2
Hoeksema, J.T.3
Harvey, K.L.4
-
20
-
-
34250488818
-
A model of interplanetary and coronal magnetic fields
-
Schatten, K. H., J. M. Wilcox, and N. F. Ness (1969), A model of interplanetary and coronal magnetic fields, Sol. Phys., 6, 442-455.
-
(1969)
Sol. Phys
, vol.6
, pp. 442-455
-
-
Schatten, K.H.1
Wilcox, J.M.2
Ness, N.F.3
-
21
-
-
39449122722
-
The heliospheric current sheet
-
Smith, E. J. (2001), The heliospheric current sheet, J. Geophys. Res., 106(AS), 15,819-15,831.
-
(2001)
J. Geophys. Res
, vol.106
, Issue.AS
-
-
Smith, E.J.1
-
22
-
-
0001627854
-
The steady global corona
-
Steinolfson, R. S., S. T. Suess, and S. T. Wu (1982), The steady global corona, Astrophys. J., 255, 730-742.
-
(1982)
Astrophys. J
, vol.255
, pp. 730-742
-
-
Steinolfson, R.S.1
Suess, S.T.2
Wu, S.T.3
-
23
-
-
44349166084
-
How good (or bad) are the inner boundary conditions for heliospheric solar wind modeling
-
Zermatt, Utah, 31 July-4 August
-
Svalgaard, L. (2006), How good (or bad) are the inner boundary conditions for heliospheric solar wind modeling, SHINE 2006 Workshop, Zermatt, Utah, 31 July-4 August.
-
(2006)
SHINE 2006 Workshop
-
-
Svalgaard, L.1
-
24
-
-
34250274743
-
The strength of the sun's polar fields
-
Svalgaard, L., T. L. Duvall Jr., and P. H. Scherrer (1978), The strength of the sun's polar fields, Sol. Phys., 58, 225-239.
-
(1978)
Sol. Phys
, vol.58
, pp. 225-239
-
-
Svalgaard, L.1
Duvall Jr., T.L.2
Scherrer, P.H.3
-
25
-
-
84905354744
-
-
Usmanov, A. V. (1996), A global 3-D MHD solar wind model with Alfvén waves, in Solar Wind Eight, edited by D. Winterhalter et al., AIP Conf. Proc.,382, 141-144.
-
Usmanov, A. V. (1996), A global 3-D MHD solar wind model with Alfvén waves, in Solar Wind Eight, edited by D. Winterhalter et al., AIP Conf. Proc.,382, 141-144.
-
-
-
-
26
-
-
39449115935
-
A global MHD solar wind model with WKB Alfvén waves: Comparison with Ulysses data
-
Usmanov, A. V., M. L. Goldstein, B. P. Besser, and J. M. Fritzer (2000), A global MHD solar wind model with WKB Alfvén waves: Comparison with Ulysses data, J. Geophys. Res., 105(AS), 12,675-12,695.
-
(2000)
J. Geophys. Res
, vol.105
, Issue.AS
-
-
Usmanov, A.V.1
Goldstein, M.L.2
Besser, B.P.3
Fritzer, J.M.4
-
27
-
-
0001545287
-
On potential field models of the solar corona
-
Wang, Y. M., and N. R. Sheeley Jr. (1992), On potential field models of the solar corona, Astrophys. J., 392, 310-319.
-
(1992)
Astrophys. J
, vol.392
, pp. 310-319
-
-
Wang, Y.M.1
Sheeley Jr., N.R.2
-
28
-
-
21744448559
-
Origin and evolution of coronal streamer structure during the 1996 minimum activity phase
-
Wang, Y. M., et al. (1997), Origin and evolution of coronal streamer structure during the 1996 minimum activity phase, Astrophys. J., 485, 875-889.
-
(1997)
Astrophys. J
, vol.485
, pp. 875-889
-
-
Wang, Y.M.1
-
29
-
-
0034353440
-
The long-term variation of the Sun's open magnetic flux
-
Wang, Y. M., J. Lean, and N. R. Sheeley Jr. (2000a), The long-term variation of the Sun's open magnetic flux, Geophys. Res. Lett., 27(4), 505-508.
-
(2000)
Geophys. Res. Lett
, vol.27
, Issue.4
, pp. 505-508
-
-
Wang, Y.M.1
Lean, J.2
Sheeley Jr., N.R.3
-
30
-
-
0034353497
-
-
Wang, Y. M., N. R. Sheeley Jr., and N. B. Rich (2000b), Evolution of coronal streamer structure during the rising phase of solar cycle 23, Geophys. Res. Lett., 27(2), 149-152.
-
Wang, Y. M., N. R. Sheeley Jr., and N. B. Rich (2000b), Evolution of coronal streamer structure during the rising phase of solar cycle 23, Geophys. Res. Lett., 27(2), 149-152.
-
-
-
-
31
-
-
0141516468
-
-
Wang, Y. M., N. R. Sheeley Jr., and M. D. Andrews (2002), Polarity reversal of the solar magnetic field during cycle 23, J. Geophys. Res., 107(A12), 1465, doi:10.1029/2002JA009463.
-
Wang, Y. M., N. R. Sheeley Jr., and M. D. Andrews (2002), Polarity reversal of the solar magnetic field during cycle 23, J. Geophys. Res., 107(A12), 1465, doi:10.1029/2002JA009463.
-
-
-
-
32
-
-
33749665535
-
Global distribution of coronal mass outputs and its relation to solar magnetic field sturctures
-
doi:10.1029/2002JA009439
-
Wei, F. S., X. S. Feng, H. C. Cai, and Q. J. Zhou (2003), Global distribution of coronal mass outputs and its relation to solar magnetic field sturctures, J. Geophys. Res., 108(A6), 1238, doi:10.1029/2002JA009439.
-
(2003)
J. Geophys. Res
, vol.108
, Issue.A6
, pp. 1238
-
-
Wei, F.S.1
Feng, X.S.2
Cai, H.C.3
Zhou, Q.J.4
-
33
-
-
0036151689
-
A space-time conservation element and solution element method for solving the two-and three-dimensional unsteady Euler equations using quadrilateral and hexahedral meshes
-
Zhang, Z. C., S. T. John Yu, and S. C. Chang (2002), A space-time conservation element and solution element method for solving the two-and three-dimensional unsteady Euler equations using quadrilateral and hexahedral meshes, J. Comput Phys., 175, 168-199.
-
(2002)
J. Comput Phys
, vol.175
, pp. 168-199
-
-
Zhang, Z.C.1
John Yu, S.T.2
Chang, S.C.3
-
34
-
-
33947540053
-
Success rate of predicting the heliospheric magnetic field polarity with Michelson Doppler Imager (MDI) synoptic charts
-
doi: 10.1029/2005JA011576
-
Zhao, X. P., J. T. Hoeksema, Y. Liu, and P. H. Scherrer (2006), Success rate of predicting the heliospheric magnetic field polarity with Michelson Doppler Imager (MDI) synoptic charts, J. Geophys. Res., 111, A10108, doi: 10.1029/2005JA011576.
-
(2006)
J. Geophys. Res
, vol.111
-
-
Zhao, X.P.1
Hoeksema, J.T.2
Liu, Y.3
Scherrer, P.H.4
|