;+ ; Project : STEREO ; ; Name : WCS_PROJ_GRA ; ; Purpose : Convert intermediate coordinates in GRA projection. ; ; Category : FITS, Coordinates, WCS ; ; Explanation : This routine is called from WCS_GET_COORD to apply the ; grism-in-air (GRA) projection to intermediate relative ; coordinates. ; ; Syntax : WCS_PROJ_GRA, WCS, COORD, I_AXIS ; ; Examples : See WCS_GET_COORD ; ; Inputs : WCS = A World Coordinate System structure, from FITSHEAD2WCS. ; COORD = The intermediate coordinates, relative to the reference ; pixel (i.e. CRVAL hasn't been applied yet). ; I_AXIS= The axis to apply the projection to. ; ; Opt. Inputs : None. ; ; Outputs : The projected coordinates are returned in the COORD array. ; ; Opt. Outputs: None. ; ; Keywords : None. ; ; Calls : TAG_EXIST, NTRIM ; ; Common : None. ; ; Restrictions: Because this routine is intended to be called only from ; WCS_GET_COORD, no error checking is performed. ; ; Side effects: None. ; ; Prev. Hist. : None. ; ; History : Version 1, 07-Jun-2005, William Thompson, GSFC ; ; Contact : WTHOMPSON ;- ; pro wcs_proj_gra, wcs, coord, i_axis on_error, 2 c = 2.99792458d8 ;Speed of light h = 6.6260693d-34 ;Planck constant param = [287.6155d0, 1.62887d-12, 0.01360d-24] pder = [287.6155d0, -1.62887d-12, -0.04080d-24] ; ; Get the grism parameters. ; g = 0.d0 if tag_exist(wcs, 'proj_names', /top_level) then begin name = 'PV' + ntrim(wcs.ix+1) + '_0' w = where(wcs.proj_names eq name, count) if count gt 0 then g = wcs.proj_values[w[0]] endif ; m = 0.d0 if tag_exist(wcs, 'proj_names', /top_level) then begin name = 'PV' + ntrim(wcs.ix+1) + '_1' w = where(wcs.proj_names eq name, count) if count gt 0 then m = wcs.proj_values[w[0]] endif ; alpha = 0.d0 if tag_exist(wcs, 'proj_names', /top_level) then begin name = 'PV' + ntrim(wcs.ix+1) + '_2' w = where(wcs.proj_names eq name, count) if count gt 0 then alpha = wcs.proj_values[w[0]] endif alpha = alpha * !dpi / 180.d0 ; nr = 1.d0 if tag_exist(wcs, 'proj_names', /top_level) then begin name = 'PV' + ntrim(wcs.ix+1) + '_3' w = where(wcs.proj_names eq name, count) if count gt 0 then nr = wcs.proj_values[w[0]] endif ; nrprime = 0.d0 if tag_exist(wcs, 'proj_names', /top_level) then begin name = 'PV' + ntrim(wcs.ix+1) + '_4' w = where(wcs.proj_names eq name, count) if count gt 0 then nrprime = wcs.proj_values[w[0]] endif ; epsilon = 0.d0 if tag_exist(wcs, 'proj_names', /top_level) then begin name = 'PV' + ntrim(wcs.ix+1) + '_5' w = where(wcs.proj_names eq name, count) if count gt 0 then epsilon = wcs.proj_values[w[0]] endif epsilon = epsilon * !dpi / 180.d0 ; theta = 0.d0 if tag_exist(wcs, 'proj_names', /top_level) then begin name = 'PV' + ntrim(wcs.ix+1) + '_6' w = where(wcs.proj_names eq name, count) if count gt 0 then theta = wcs.proj_values[w[0]] endif theta = theta * !dpi / 180.d0 ; ; Simplify into the independent variables. ; gme = g * m / cos(epsilon) nra = nr * sin(alpha) nraprime = nrprime * sin(alpha) ; ; Get the final variable type. ; coord_type = strupcase( strmid(wcs.ctype[i_axis], 0, 4) ) ; ; Parse the units specification. ; cunit = wcs.cunit[i_axis] wcs_parse_units, cunit, base_units, factor ; ; Get the reference wavelength, and the derivative needed to calculate ; dGamma/dw at the reference point. The distinction between vacuum and air ; wavelengths will be handled further down. ; case coord_type of 'FREQ': begin if (base_units ne 's^-1') and (cunit ne '') then begin message = 'Illegal units specification ' + cunit goto, handle_error endif nu0 = factor * wcs.crval[i_axis] lambda0 = c / nu0 deriv = -c / nu0^2 end 'ENER': begin if (base_units ne 'kg.m^2.s^-2') and (cunit ne '') then begin message = 'Illegal units specification ' + cunit goto, handle_error endif nu0 = factor * wcs.crval[i_axis] / h lambda0 = c / nu0 deriv = -c * h / nu0^2 endcase 'WAVN': begin if (base_units ne 'm^-1') and (cunit ne '') then begin message = 'Illegal units specification ' + cunit goto, handle_error endif kappa0 = factor * wcs.crval[i_axis] lambda0 = 1.d0 / kappa0 deriv = -1.d0 / (c * kappa0)^2 endcase 'VRAD': begin if (base_units ne 'm.s^-1') and (cunit ne '') then begin message = 'Illegal units specification ' + cunit goto, handle_error endif restfrq = 0 if tag_exist(wcs,'spectrum') then begin if tag_exist(wcs.spectrum, 'RESTFRQ') then $ restfrq = wcs.spectrum.restfrq endif if restfrq eq 0 then begin message = 'Rest frequency not available -- ignoring projection' goto, handle_error endif v0 = factor * wcs.crval[i_axis] nu0 = restfrq * (1.d0 - v0 / c) lambda0 = c / nu0 deriv = restfrq / nu0^2 endcase 'WAVE': begin if (base_units ne 'm') and (cunit ne '') then begin message = 'Illegal units specification ' + cunit goto, handle_error endif lambda0 = factor * wcs.crval[i_axis] deriv = 1.d0 endcase 'VOPT': begin if (base_units ne 'm.s^-1') and (cunit ne '') then begin message = 'Illegal units specification ' + cunit goto, handle_error endif restwav = 0 if tag_exist(wcs,'spectrum') then begin if tag_exist(wcs.spectrum, 'RESTWAV') then $ restwav=wcs.spectrum.restwav endif if restwav eq 0 then begin message = 'Rest wavelength not available -- ignoring projection' goto, handle_error endif z0 = factor * wcs.crval[i_axis] lambda0 = restwav * (1.d0 + z0 / c) deriv = restwav / c endcase 'ZOPT': begin if (base_units ne '') and (cunit ne '') then begin message = 'Illegal units specification ' + cunit goto, handle_error endif restwav = 0 if tag_exist(wcs,'spectrum') then begin if tag_exist(wcs.spectrum, 'RESTWAV') then $ restwav=wcs.spectrum.restwav endif if restwav eq 0 then begin message = 'Rest wavelength not available -- ignoring projection' goto, handle_error endif z0 = factor * wcs.crval[i_axis] lambda0 = restwav * (1.d0 + z0) deriv = restwav endcase 'AWAV': begin if (base_units ne 'm') and (cunit ne '') then begin message = 'Illegal units specification ' + cunit goto, handle_error endif lambda0 = factor * wcs.crval[i_axis] deriv = 1.d0 endcase 'VELO': begin if (base_units ne 'm.s^-1') and (cunit ne '') then begin message = 'Illegal units specification ' + cunit goto, handle_error endif restwav = 0 if tag_exist(wcs,'spectrum') then begin if tag_exist(wcs.spectrum, 'RESTWAV') then $ restwav=wcs.spectrum.restwav endif if restwav eq 0 then begin message = 'Rest wavelength not available -- ignoring projection' goto, handle_error endif v0 = factor * wcs.crval[i_axis] lambda0 = restwav * (c + v0) / sqrt(c^2 - v0^2) deriv = c * restwav / ((c - v0) * sqrt(c^2 - v0^2)) end 'BETA': begin if (base_units ne '') and (cunit ne '') then begin message = 'Illegal units specification ' + cunit goto, handle_error endif restwav = 0 if tag_exist(wcs,'spectrum') then begin if tag_exist(wcs.spectrum, 'RESTWAV') then $ restwav=wcs.spectrum.restwav endif if restwav eq 0 then begin message = 'Rest wavelength not available -- ignoring projection' goto, handle_error endif v0 = factor * wcs.crval[i_axis] * c lambda0 = restwav * (c + v0) / sqrt(c^2 - v0^2) deriv = c^2 * restwav / ((c - v0) * sqrt(c^2 - v0^2)) endcase else: begin message = 'Invalid projection ' + wcs.ctype[i_axis] + ' -- ignored' goto, handle_error endcase endcase ; ; Unless the coordinate type is AWAV, correct for the distinction between ; vacuum and air wavelengths. ; if coord_type ne 'AWAV' then begin lambda0 = lambda0 / $ (1.d0 + 1.d-6 * (param[0] + param[1]/lambda0^2 + param[2]/lambda0^4)) deriv = deriv * $ (1.d0 + 1.d-6 * (pder[0] + pder[1]/lambda0^2 + pder[2]/lambda0^4)) endif ; ; Calculate the reference angle gamma_r, and the derivative dGamma/dw. ; gamma0 = gme * lambda0 - nra if abs(gamma0) le 1 then gamma0 = asin(gamma0) else begin message = 'Incompatible grism parameters -- not projecting' goto, handle_error endelse denom = cos(gamma0) * cos(theta)^2 if denom eq 0 then begin message = 'Incompatible grism parameters -- not projecting' goto, handle_error endif dgdw = deriv * (gme - nraprime) / denom ; ; Calculate the grism parameter, and use it to calculate the wavelength. ; gamma = -tan(theta) + dgdw * factor * coord[i_axis,*] gamma = atan(gamma) + gamma0 + theta denom = gme - nraprime if denom eq 0 then begin message = 'Incompatible grism parameters -- not projecting' goto, handle_error endif lambda = (nra - nraprime * lambda0 + sin(gamma)) / denom ; ; Unless the coordinate type is AWAV, correct for the distinction between ; vacuum and air wavelengths. ; if coord_type ne 'AWAV' then lambda = lambda * $ (1.d0 + 1.d-6 * (param[0] + param[1]/lambda^2 + param[2]/lambda^4)) ; ; Convert into the final spectral coordinate variable. ; case coord_type of 'FREQ': s = c / lambda 'ENER': s = h * c / lambda 'WAVN': s = 1.d0 / lambda 'VRAD': begin freq = c / lambda s = c * (restfrq - freq) / restfrq endcase 'WAVE': s = lambda 'VOPT': s = c * (lambda - restwav) / restwav 'ZOPT': s = (lambda - restwav) / restwav 'AWAV': s = lambda 'VELO': s = c * (lambda^2 - restwav^2) / (lambda^2 + restwav^2) 'BETA': s = (lambda^2 - restwav^2) / (lambda^2 + restwav^2) endcase ; ; Apply the appropriate units conversion, and return. ; coord[i_axis,*] = s / factor return ; ; Error handling point. ; handle_error: message, message, /continue coord[i_axis,*] = coord[i_axis,*] + wcs.crval[i_axis] ; return end