We explain two puzzling aspects of Petschek's model for fast reconnection. One is its failure to occur in plasma simulations with uniform resistivity. The other is its inability to provide anything more than an upper limit for the reconnection rate. We have found that previously published analytical solutions based on Petschek's model are structurally unstable if the electrical resistivity is uniform. The structural instability is associated with the presence of an essential singularity at the X-line that is unphysical. By requiring that such a singularity does not exist, we obtain a formula that predicts a specific rate of reconnection. For uniform resistivity, reconnection can only occur at the slow, Sweet-Parker rate. For nonuniform resistivity, reconnection can occur at a much faster rate provided that the resistivity profile is not too flat near the X-line. If this condition is satisfied, then the scale length of the nonuniformity determines the reconnection rate.

1.
H. E.
Petschek
, in
The Physics of Solar Flares
, edited by
W. N.
Hess
(
NASA, SP-50
,
1964
), p.
425
.
2.
M.
Yan
,
L. C.
Lee
, and
E. R.
Priest
,
J. Geophys. Res.
97
,
8277
, doi: (
1992
).
3.
D. A.
Uzdensky
and
R. M.
Kulsrud
,
Phys. Plasmas
7
,
4018
(
2000
).
4.
M.
Ugai
,
Plasma Phys. Controlled Fusion
26
,
1549
(
1984
).
5.
M.
Scholer
,
Geophys. Astrophys. Fluid Dyn.
62
,
51
(
1991
).
6.
N. V.
Erkaev
,
V. S.
Semenov
, and
H. K.
Biernat
,
Nonlinear Processes Geophys.
9
,
131
(
2002
).
7.
H.
Baty
,
T. G.
Forbes
, and
E. R.
Priest
,
Phys. Plasmas
16
,
012102
(
2009
).
8.
H.
Baty
,
E. R.
Priest
, and
T. G.
Forbes
,
Phys. Plasmas
16
,
060701
(
2009
).
9.
B.
Roberts
and
E. R.
Priest
,
J. Plasma Phys.
14
,
417
(
1975
).
10.
T. G.
Forbes
and
E. R.
Priest
,
Rev. Geophys.
25
,
1583
, doi: (
1987
).
11.
E. N.
Parker
,
J. Geophys. Res.
62
,
509
, doi: (
1957
).
12.
A. M.
Soward
and
E. R.
Priest
,
Philos. Trans. R. Soc. London, Ser. A
284
,
369
(
1977
).
13.
L. M.
Malyshkin
,
T.
Linde
, and
R. M.
Kulsrud
,
Phys. Plasmas
12
,
102902
(
2005
).
14.
L. M.
Malyshkin
and
R. M.
Kulsrud
,
Phys. Scr.
T142
,
014034
(
2010
).
15.
R. M.
Kulsrud
,
Phys. Plasmas
18
,
111201
(
2011
).
16.
V. M.
Vasyliunas
,
Rev. Geophys.
13
,
303
, doi: (
1975
).
17.
B. V.
Somov
,
V. S.
Titov
, and
A. I.
Verneta
,
Itogi Nauki Tekh. Ser. Astron.
34
,
136
(
1987
) (in Russian).
18.
B. V.
Somov
,
Physical Processes in Solar Flares
(
Kluwer
,
Dordrecht
,
1992
).
19.
V. S.
Titov
, in
Physics of Solar Flares
, edited by
B. V.
Somov
(
IZMIRAN
,
Moscow
,
1985
), p.
141
.
20.
V. S.
Titov
, “
Magnetic reconnection in a high-temperature solar plasma
,” M.S. thesis (
Moscow Institute of Physics and Technology
,
1985
) (in Russian).
21.
B. V.
Somov
,
Plasma Astrophysics Part I: Fundamentals and Practice
(
Spinger
,
New York
,
2006
).
22.
R. M.
Green
, in
Solar and Stellar Magnetic fields
, edited by
R.
Lüst
(
North-Holland Publishing Co.
,
Amsterdam
,
1965
), p.
398
.
23.
S. I.
Syrovatskii
,
Sov. Phys. JETP
33
,
933
(
1971
) (Engl. Transl.).
24.
D. B.
Seaton
and
T. G.
Forbes
,
Astrophys. J.
701
,
348
(
2009
).
25.
K.
Liffman
,
Publ. - Astron. Soc. Aust.
18
,
267
(
2001
).
26.
R. D.
Blandford
and
M. J.
Rees
,
Mon. Not. R. Astron. Soc.
169
,
395
(
1974
).
27.
S.-H.
Kim
and
A. C.
Raga
,
Astrophys. J.
379
,
689
(
1991
).
28.
H.
Baty
,
E. R.
Priest
, and
T. G.
Forbes
,
Phys. Plasmas
13
,
022312
(
2006
).
29.
E. R.
Priest
and
T. G.
Forbes
,
Magnetic Reconnection: MHD Theory and Applications
(
Cambridge University Press
,
Cambridge
,
2000
).
30.
E. R.
Priest
and
T. G.
Forbes
,
J. Geophys. Res.
91
,
5579
, doi: (
1986
).
31.
N. A.
Murphy
and
C. R.
Sovinec
,
Phys. Plasmas
15
,
042313
(
2008
).
32.
S.
Schreier
,
Compressible Flow
(
Wiley
,
New York
,
1982
).
You do not currently have access to this content.