use precinput.asc for clarity

space-physics · May 20, 2020 · 6e212f9 · 6e212f9
1 parent f90e500
commit 6e212f9
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Showing 2 changed files with 8 additions and 8 deletions.
diff --git a/DATCAR_spectrum.asc b/DATCAR_spectrum.asc
@@ -1,12 +1,12 @@
 2					(kiappel, INTEGER)
-conttanh.dat                                input file (initial ionospheric conditions) leave this many spaces separating
+conttanh.dat                       input file (initial ionospheric conditions) leave this many spaces separating
 1.					time step (seconds) (REAL)
-1.				number of seconds between fluid code outputs (seconds, REAL)
-2013090					date of simulation (YYYYDDD)
+1.		                     number of seconds between fluid code outputs (seconds, REAL)
+2013090			       date of simulation (YYYYDDD)
 32419.					UT start time for simulation (seconds)
 300.					duration of run (seconds)
 2					jpreci, precipation type (see table below, INTEGER)
-65.12,-147.43    				location of simulation, geodetic latitude,longitude
+65.12,-147.43    			location of simulation, geodetic latitude,longitude
 0.					duration of convection (in seconds) before the reference (<= 0, we do not follow the field lines)  (tempsconv_1, REAL)
 0.					duration of convection (in seconds) before the reference (<= 0, we do not follow the field lines)  (tempsconv, REAL)
 0					time interval (seconds) between two tubes (step,REAL)
@@ -22,7 +22,7 @@ conttanh.dat                                input file (initial ionospheric cond
 1.					N correction factor (REAL)
 1.					H correction factor (REAL)
 -1.e-4					topside electron heat flux (mW/m^2, REAL)
-precinput.dat   	                electron precipitation distribution file (energy (eV) in first column, number flux (cm^-2 s^-1 eV^-1 sr^-1) in second column)
+precinput.asc                      electron precipitation distribution file (energy (eV) in first column, number flux (cm^-2 s^-1 eV^-1 sr^-1) in second column)
 1					precint, precipation energy interpolation (see table below, INTEGER)
 1					precext, precipation energy extrapolation (see table below, INTEGER)
 32460.					precipitation start time (seconds from day start)

diff --git a/transcar/io.py b/transcar/io.py
@@ -19,7 +19,7 @@
 FOK = "finish.status"
 
 
-PREC = "dir.input/precinput.dat"  # NOT based on root, MUST be relative!!
+PREC = "dir.input/precinput.asc"  # NOT based on root, MUST be relative!!
 
 
 def cp_parents(files: T.Sequence[Path], target_dir: Path, origin: Path = None) -> None:
@@ -124,7 +124,7 @@ def setup_dirs(odir: Path, params: T.Dict[str, T.Any]) -> T.Tuple[T.Dict[str, T.
 
 def setup_monoprec(odir: Path, inp: T.Dict[str, T.Any], beam: T.Dict[str, float], flux0: float) -> None:
     """
-    write dir.input/precinput.dat for monoenergetic beam case
+    write dir.input/precinput.asc for monoenergetic beam case
     """
     ofn = Path(odir).expanduser() / PREC
 
@@ -148,7 +148,7 @@ def setup_monoprec(odir: Path, inp: T.Dict[str, T.Any], beam: T.Dict[str, float]
 
 def setup_spectrum_prec(odir: Path, inp: T.Dict[str, T.Any], beam: pandas.DataFrame) -> None:
     """
-    write dir.input/precinput.dat for beam with shaped differential number flux
+    write dir.input/precinput.asc for beam with shaped differential number flux
     """
     ofn = Path(odir).expanduser() / PREC