version 1.34, 2015/02/27 19:49:43
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version 1.38, 2020/06/30 22:38:17
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/*=========================================== | /*=========================================== |
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The following 14 functions calculate the following spaceweather indices: | The following 14 functions calculate the following spaceweather indices: |
Line 280 int computeBtotalderivative(float *bt, i |
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Line 281 int computeBtotalderivative(float *bt, i |
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} | } |
} | } |
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/* consider the edges for the arrays that contribute to the variable "sum" in the computation below. |
/* consider the edges */ |
ignore the edges for the error terms as those arrays have been initialized to zero. |
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this is okay because the error term will ultimately not include the edge pixels as they are selected out by the mask and bitmask arrays.*/ |
i=0; | i=0; |
for (j = 0; j <= ny-1; j++) | for (j = 0; j <= ny-1; j++) |
{ | { |
Line 374 int computeBhderivative(float *bh, float |
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Line 376 int computeBhderivative(float *bh, float |
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} | } |
} | } |
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/* consider the edges for the arrays that contribute to the variable "sum" in the computation below. |
/* consider the edges */ |
ignore the edges for the error terms as those arrays have been initialized to zero. |
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this is okay because the error term will ultimately not include the edge pixels as they are selected out by the mask and bitmask arrays.*/ |
i=0; | i=0; |
for (j = 0; j <= ny-1; j++) | for (j = 0; j <= ny-1; j++) |
{ | { |
Line 468 int computeBzderivative(float *bz, float |
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Line 471 int computeBzderivative(float *bz, float |
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} | } |
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/* consider the edges for the arrays that contribute to the variable "sum" in the computation below. | /* consider the edges for the arrays that contribute to the variable "sum" in the computation below. |
ignore the edges for err_termA and err_term B as those arrays have been initialized to zero. |
ignore the edges for the error terms as those arrays have been initialized to zero. |
this is okay because the error term will ultimately not include the edge pixels as they are selected out by the mask and bitmask arrays.*/ | this is okay because the error term will ultimately not include the edge pixels as they are selected out by the mask and bitmask arrays.*/ |
i=0; | i=0; |
for (j = 0; j <= ny-1; j++) | for (j = 0; j <= ny-1; j++) |
Line 595 int computeJz(float *bx_err, float *by_e |
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Line 598 int computeJz(float *bx_err, float *by_e |
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} | } |
} | } |
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// consider the edges |
/* consider the edges for the arrays that contribute to the variable "sum" in the computation below. |
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ignore the edges for the error terms as those arrays have been initialized to zero. |
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this is okay because the error term will ultimately not include the edge pixels as they are selected out by the mask and bitmask arrays.*/ |
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i=0; | i=0; |
for (j = 0; j <= ny-1; j++) | for (j = 0; j <= ny-1; j++) |
{ | { |
derx[j * nx + i] = ( (-3*by[j * nx + i]) + (4*by[j * nx + (i+1)]) - (by[j * nx + (i+2)]) )*0.5; | derx[j * nx + i] = ( (-3*by[j * nx + i]) + (4*by[j * nx + (i+1)]) - (by[j * nx + (i+2)]) )*0.5; |
err_term1[j * nx + i] = ( (3*by_err[j * nx + i])*(3*by_err[j * nx + i]) + (4*by_err[j * nx + (i+1)])*(4*by_err[j * nx + (i+1)]) + (by_err[j * nx + (i+2)])*(by_err[j * nx + (i+2)]) ); |
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} | } |
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i=nx-1; | i=nx-1; |
for (j = 0; j <= ny-1; j++) | for (j = 0; j <= ny-1; j++) |
{ | { |
derx[j * nx + i] = ( (3*by[j * nx + i]) + (-4*by[j * nx + (i-1)]) - (-by[j * nx + (i-2)]) )*0.5; | derx[j * nx + i] = ( (3*by[j * nx + i]) + (-4*by[j * nx + (i-1)]) - (-by[j * nx + (i-2)]) )*0.5; |
err_term1[j * nx + i] = ( (3*by_err[j * nx + i])*(3*by_err[j * nx + i]) + (4*by_err[j * nx + (i+1)])*(4*by_err[j * nx + (i+1)]) + (by_err[j * nx + (i+2)])*(by_err[j * nx + (i+2)]) ); |
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} | } |
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j=0; | j=0; |
for (i = 0; i <= nx-1; i++) | for (i = 0; i <= nx-1; i++) |
{ | { |
dery[j * nx + i] = ( (-3*bx[j*nx + i]) + (4*bx[(j+1) * nx + i]) - (bx[(j+2) * nx + i]) )*0.5; | dery[j * nx + i] = ( (-3*bx[j*nx + i]) + (4*bx[(j+1) * nx + i]) - (bx[(j+2) * nx + i]) )*0.5; |
err_term2[j * nx + i] = ( (3*bx_err[j*nx + i])*(3*bx_err[j*nx + i]) + (4*bx_err[(j+1) * nx + i])*(4*bx_err[(j+1) * nx + i]) + (bx_err[(j+2) * nx + i])*(bx_err[(j+2) * nx + i]) ); |
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} | } |
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j=ny-1; | j=ny-1; |
for (i = 0; i <= nx-1; i++) | for (i = 0; i <= nx-1; i++) |
{ | { |
dery[j * nx + i] = ( (3*bx[j * nx + i]) + (-4*bx[(j-1) * nx + i]) - (-bx[(j-2) * nx + i]) )*0.5; | dery[j * nx + i] = ( (3*bx[j * nx + i]) + (-4*bx[(j-1) * nx + i]) - (-bx[(j-2) * nx + i]) )*0.5; |
err_term2[j * nx + i] = ( (3*bx_err[j*nx + i])*(3*bx_err[j*nx + i]) + (4*bx_err[(j+1) * nx + i])*(4*bx_err[(j+1) * nx + i]) + (bx_err[(j+2) * nx + i])*(bx_err[(j+2) * nx + i]) ); |
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} | } |
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Line 830 int computeHelicity(float *jz_err, float |
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Line 831 int computeHelicity(float *jz_err, float |
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/* Example function 12: Sum of Absolute Value per polarity */ | /* Example function 12: Sum of Absolute Value per polarity */ |
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// The Sum of the Absolute Value per polarity is defined as the following: | // The Sum of the Absolute Value per polarity is defined as the following: |
// fabs(sum(jz gt 0)) + fabs(sum(jz lt 0)) and the units are in Amperes per arcsecond. |
// fabs(sum(jz gt 0)) + fabs(sum(jz lt 0)) and the units are in Amperes per square arcsecond. |
// The units of jz are in G/pix. In this case, we would have the following: | // The units of jz are in G/pix. In this case, we would have the following: |
// Jz = (Gauss/pix)(1/CDELT1)(0.00010)(1/MUNAUGHT)(RSUN_REF/RSUN_OBS)(RSUN_REF/RSUN_OBS)(RSUN_OBS/RSUN_REF), | // Jz = (Gauss/pix)(1/CDELT1)(0.00010)(1/MUNAUGHT)(RSUN_REF/RSUN_OBS)(RSUN_REF/RSUN_OBS)(RSUN_OBS/RSUN_REF), |
// = (Gauss/pix)(1/CDELT1)(0.00010)(1/MUNAUGHT)(RSUN_REF/RSUN_OBS) | // = (Gauss/pix)(1/CDELT1)(0.00010)(1/MUNAUGHT)(RSUN_REF/RSUN_OBS) |
Line 1233 int computeLorentz(float *bx, float *by |
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Line 1234 int computeLorentz(float *bx, float *by |
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} | } |
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/*===========================================*/ |
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/* Example function 17: Compute total unsigned flux in units of G/cm^2 on the LOS field */ |
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// To compute the unsigned flux, we simply calculate |
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// flux = surface integral [(vector LOS) dot (normal vector)], |
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// = surface integral [(magnitude LOS)*(magnitude normal)*(cos theta)]. |
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// However, since the field is radial, we will assume cos theta = 1. |
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// Therefore the pixels only need to be corrected for the projection. |
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// To convert G to G*cm^2, simply multiply by the number of square centimeters per pixel. |
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// As an order of magnitude estimate, we can assign 0.5 to CDELT1 and 722500m/arcsec to (RSUN_REF/RSUN_OBS). |
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// (Gauss/pix^2)(CDELT1)^2(RSUN_REF/RSUN_OBS)^2(100.cm/m)^2 |
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// =Gauss*cm^2 |
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int computeAbsFlux_los(float *los, int *dims, float *absFlux, |
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float *mean_vf_ptr, float *count_mask_ptr, |
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int *bitmask, float cdelt1, double rsun_ref, double rsun_obs) |
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{ |
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int nx = dims[0]; |
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int ny = dims[1]; |
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int i = 0; |
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int j = 0; |
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int count_mask = 0; |
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double sum = 0.0; |
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*absFlux = 0.0; |
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*mean_vf_ptr = 0.0; |
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if (nx <= 0 || ny <= 0) return 1; |
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for (i = 0; i < nx; i++) |
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{ |
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for (j = 0; j < ny; j++) |
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{ |
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if ( bitmask[j * nx + i] < 30 ) continue; |
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if isnan(los[j * nx + i]) continue; |
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sum += (fabs(los[j * nx + i])); |
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count_mask++; |
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} |
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} |
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*mean_vf_ptr = sum*cdelt1*cdelt1*(rsun_ref/rsun_obs)*(rsun_ref/rsun_obs)*100.0*100.0; |
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*count_mask_ptr = count_mask; |
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return 0; |
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} |
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/*===========================================*/ |
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/* Example function 18: Derivative of B_LOS (approximately B_vertical) = SQRT( ( dLOS/dx )^2 + ( dLOS/dy )^2 ) */ |
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int computeLOSderivative(float *los, int *dims, float *mean_derivative_los_ptr, int *bitmask, float *derx_los, float *dery_los) |
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{ |
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int nx = dims[0]; |
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int ny = dims[1]; |
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int i = 0; |
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int j = 0; |
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int count_mask = 0; |
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double sum = 0.0; |
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*mean_derivative_los_ptr = 0.0; |
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if (nx <= 0 || ny <= 0) return 1; |
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/* brute force method of calculating the derivative (no consideration for edges) */ |
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for (i = 1; i <= nx-2; i++) |
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{ |
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for (j = 0; j <= ny-1; j++) |
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{ |
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derx_los[j * nx + i] = (los[j * nx + i+1] - los[j * nx + i-1])*0.5; |
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} |
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} |
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/* brute force method of calculating the derivative (no consideration for edges) */ |
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for (i = 0; i <= nx-1; i++) |
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{ |
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for (j = 1; j <= ny-2; j++) |
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{ |
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dery_los[j * nx + i] = (los[(j+1) * nx + i] - los[(j-1) * nx + i])*0.5; |
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} |
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} |
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/* consider the edges for the arrays that contribute to the variable "sum" in the computation below. |
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ignore the edges for the error terms as those arrays have been initialized to zero. |
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this is okay because the error term will ultimately not include the edge pixels as they are selected out by the mask and bitmask arrays.*/ |
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i=0; |
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for (j = 0; j <= ny-1; j++) |
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{ |
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derx_los[j * nx + i] = ( (-3*los[j * nx + i]) + (4*los[j * nx + (i+1)]) - (los[j * nx + (i+2)]) )*0.5; |
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} |
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i=nx-1; |
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for (j = 0; j <= ny-1; j++) |
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{ |
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derx_los[j * nx + i] = ( (3*los[j * nx + i]) + (-4*los[j * nx + (i-1)]) - (-los[j * nx + (i-2)]) )*0.5; |
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} |
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j=0; |
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for (i = 0; i <= nx-1; i++) |
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{ |
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dery_los[j * nx + i] = ( (-3*los[j*nx + i]) + (4*los[(j+1) * nx + i]) - (los[(j+2) * nx + i]) )*0.5; |
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} |
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j=ny-1; |
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for (i = 0; i <= nx-1; i++) |
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{ |
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dery_los[j * nx + i] = ( (3*los[j * nx + i]) + (-4*los[(j-1) * nx + i]) - (-los[(j-2) * nx + i]) )*0.5; |
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} |
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for (i = 0; i <= nx-1; i++) |
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{ |
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for (j = 0; j <= ny-1; j++) |
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{ |
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if ( bitmask[j * nx + i] < 30 ) continue; |
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if ( (derx_los[j * nx + i] + dery_los[j * nx + i]) == 0) continue; |
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if isnan(los[j * nx + i]) continue; |
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if isnan(los[(j+1) * nx + i]) continue; |
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if isnan(los[(j-1) * nx + i]) continue; |
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if isnan(los[j * nx + i-1]) continue; |
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if isnan(los[j * nx + i+1]) continue; |
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if isnan(derx_los[j * nx + i]) continue; |
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if isnan(dery_los[j * nx + i]) continue; |
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sum += sqrt( derx_los[j * nx + i]*derx_los[j * nx + i] + dery_los[j * nx + i]*dery_los[j * nx + i] ); /* Units of Gauss */ |
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count_mask++; |
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} |
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} |
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*mean_derivative_los_ptr = (sum)/(count_mask); // would be divided by ((nx-2)*(ny-2)) if shape of count_mask = shape of magnetogram |
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//printf("mean_derivative_los_ptr=%f\n",*mean_derivative_los_ptr); |
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return 0; |
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} |
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/*==================KEIJI'S CODE =========================*/ | /*==================KEIJI'S CODE =========================*/ |
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// #include <omp.h> | // #include <omp.h> |