const float SST3diff2

const float SSTvdiff

PairOfVars(size_t npix)

float tg_sen[NBANDS]

an array had not been initialized Several spelling and grammar corrections were which is read from the appropriate MCF the above metadata values were hard coded A problem calculating the average background DN for SWIR bands when the moon is in the space view port was corrected The new algorithm used to calculate the average background DN for all reflective bands when the moon is in the space view port is now the same as the algorithm employed by the thermal bands For non SWIR changes in the averages are typically less than Also for non SWIR the black body DNs remain a backup in case the SV DNs are not available For SWIR the changes in computed averages were larger because the old which used the black body suffered from contamination by the micron leak As a consequence of the if SV DNs are not available for the SWIR the EV pixels will not be the granule time is used to identify the appropriate tables within the set given for one LUT the first two or last two tables respectively will be used for the interpolation If there is only one LUT in the set of it will be treated as a constant LUT The manner in which Earth View data is checked for saturation was changed Previously the raw Earth View DNs and Space View DNs were checked against the lookup table values contained in the table dn_sat The change made is to check the raw Earth and Space View DNs to be sure they are less than the maximum saturation value and to check the Space View subtracted Earth View dns against a set of values contained in the new lookup table dn_sat_ev The metadata configuration and ASSOCIATEDINSTRUMENTSHORTNAME from the MOD02HKM product The same metatdata with extensions and were removed from the MOD021KM and MOD02OBC products ASSOCIATEDSENSORSHORTNAME was set to MODIS in all products These changes are reflected in new File Specification which users may consult for exact the pow functions were eliminated in Emissive_Cal and Emissive bands replaced by more efficient code Other calculations throughout the code were also made more efficient Aside from a few round off there was no difference to the product The CPU time decreased by about for a day case and for a night case A minor bug in calculating the uncertainty index for emissive bands was corrected The frame index(0-based) was previously being used the frame number(1-based) should have been used. There were only a few minor changes to the uncertainty index(maximum of 1 digit). 3. Some inefficient arrays(Sigma_RVS_norm_sq) were eliminated and some code lines in Preprocess_L1A_Data were moved into Process_OBCEng_Emiss. There were no changes to the product. Required RAM was reduced by 20 MB. Now

const get_valid rho_mask

const float Btmax40

const float Bt12unif2

size_t npix

std::vector< float > stdv

float

std::vector< float > var_min_box

Stats(size_t npix, size_t nscan, size_t rad_x, size_t rad_y, size_t center, l1qstr *l1qrec)

int32_t day

std::vector< int16_t > counts_out

const float dBtmax

int ib

bool(* get_valid)(const l1str &, int, int, int)

void get_ratio(l1str &l1str)

const float cldthresh

float * sst1

#define NBANDSIR

std::vector< float > senz

key

These are used to scale the SD before writing it to the HDF4 file The default is and which means the product is not scaled at all Since the product is usually stored as a float inside of this is a way to write the float out as a integer l2prod min

const float SSTmaxn

const float dBt4min

int ib1

transform

int current_scan

size_t rad_y

const std::unordered_map< int, std::string > platforms

void get_window_1D_min(float *mins_1d, const float *inp1d, const int *mask1d, size_t npix, size_t radius)

const std::unordered_map< std::string, const std::unordered_map< std::string, int > > bands_set

no change in intended resolving MODur00064 Corrected handling of bad ephemeris attitude resolving resolving GSFcd00179 Corrected handling of fill values for[Sensor|Solar][Zenith|Azimuth] resolving MODxl01751 Changed to validate LUT version against a value retrieved from the resolving MODxl02056 Changed to calculate Solar Diffuser angles without adjustment for estimated post launch changes in the MODIS orientation relative to incidentally resolving defects MODxl01766 Also resolves MODxl01947 Changed to ignore fill values in SCI_ABNORM and SCI_STATE rather than treating them as resolving MODxl01780 Changed to use spacecraft ancillary data to recognise when the mirror encoder data is being set by side A or side B and to change calculations accordingly This removes the need for seperate LUTs for Side A and Side B data it makes the new LUTs incompatible with older versions of the and vice versa Also resolves MODxl01685 A more robust GRing algorithm is being which will create a non default GRing anytime there s even a single geolocated pixel in a granule Removed obsolete messages from seed as required for compatibility with version of the SDP toolkit Corrected test output file names to end in out

StatsSST()

std::vector< float > qual

float(* get_value)(const l1str &, int, int, int)

const float equatorialSouth

const float equatorialWest

read l1rec

#define VIIRSN

PairOfSST(size_t npix, float *sst1, float *sst2, bool has_difference)

const std::unordered_set< int > viirs_sensors

void read_sst_bands(const std::string &sat, std::unordered_map< std::string, int > &bands)

StatsSST(size_t npix, size_t nscan, size_t rad_x, size_t rad_y, size_t center, l1qstr *l1qrec, float *sst, bool std_requested=false, bool max_req=false, bool min_req=false, bool min_max_req=false)

product_types

#define MODIST

size_t nquar

std::ostream & operator<<(std::ostream &stream, const std::vector< T > &data)

size_t center

const float vhisenzv2

const float vhisenz

size_t nsst

const float Bt11unif2

const float SST4diff2

int * get_valid_mask()

std::vector< float > difference

const float equatorialEast

void rearrange()

size_t i_e

StatsVarBand(size_t npix, size_t nscan, size_t rad_x, size_t rad_y, size_t center, l1qstr *l1qrec, int ib, size_t nbands, cldmsk::get_valid get_mask, cldmsk::get_value get_val, bool std_requested=false, bool max_requested=false, bool min_requested=false, bool min_max_requested=false)

std::string get_ocdata_root()

std::vector< float > var_max_box

std::vector< float > lat

size_t i_s

@ string

std::vector< int16_t > counts

const get_value cirrus_value

size_t npix

solz

size_t nday

instr * input

#define M_PI

const float SST3diff1

#define BT_HI

std::vector< float > bias_mean_out

const float Bt39unif2

PairOfVarsBT()

std::string get_sensor(int key)

const std::unordered_map< std::string, std::string(*)(const instr *)> get_sses_coeffs_path

const float SSTdiff

void set_std()

float * operator()(const std::string &key)

float offset

float * sst2

float * get_Tdeflong()

size_t nlat

Stats()

size_t rad_x

PairOfVars()

const get_valid cldrh_mask

int

const float SSTmax

size_t npix

const float dBtmin

const double scan_time_modis_t_day2

const std::unordered_map< std::string, float > cldthresh_list

@ SST4

std::vector< float > bias_mean

const float min_bt

const float Bt39unif1

void calculate_sses_bias_stats(const float *diff, const float *sst, const float *solz, const float *senz, size_t day, const float *lat, const int8_t *qual, const int16_t *flags, const float *glint)

float * operator()()

std::vector< float > var_max

#define SSTF_BTNONUNIF

#define SSTF_HISENZ

const float el_corr_modis_t_1

void get_window_1D_max(float *maxs_1d, const float *inp1d, const int *mask1d, size_t npix, size_t radius)

const get_value cldrh_value

float tg_sol[NBANDS]

std::vector< float > stdv_out

std::vector< float > var_std

const float invalid_val

const get_value rho_value

const float solznight

void get_difference()

const float Btmin

std::vector< float > sst

const get_valid bt_mask

@ SST3

a context in which it is NOT documented to do so subscript which cannot be easily calculated when extracting TONS attitude data from the Terra L0 files Corrected several defects in extraction of entrained ephemeris and and as HDF file for both the L1A and Geolocation enabling retrieval of South Polar DEM data Resolved Bug by changing to opent the geolocation file only after a successful read of the L1A and also by checking for fatal errors from not restoring C5 and to report how many of those high resolution values were water in the new WaterPresent SDS Added valid_range attribute to Land SeaMask Changed to bilinearly interpolate the geoid_height to remove artifacts at one degree lines Made corrections to const qualification of pointers allowed by new version of M API library Removed casts that are no longer for same not the geoid Corrected off by one error in calculation of high resolution offsets Corrected parsing of maneuver list configuration parameter Corrected to set Height SDS to fill values when geolocation when for elevation and land water mask

const std::unordered_map< std::string, size_t > bt_box_sizes

const float max_lt

void get_difference(l1str &l1str)

void get_total_2d_min(float *min_global, const float *inp2d, size_t npix, size_t nscan, size_t center, size_t radius)

const float max_bt

@ SST

this program makes no use of any feature of the SDP Toolkit that could generate such a then geolocation is calculated at that and then aggregated up to Resolved feature request Bug by adding three new int8 SDSs for each high resolution pixel

StatsVarBand()

PairOfVarsBT(size_t npix, int ib1, int ib2, l1str &l1str, bool has_difference=false, bool has_ratio=false)

size_t nqual

const float equatorialNorth

const float SSTmin

no change in intended resolving MODur00064 Corrected handling of bad ephemeris attitude data

const float dBtrefmin

size_t nscan

const float Bt11unif1

std::vector< float > var_min

std::vector< float > & month_data()

PairOfSST()

const float SST4diff1

SSESData(const std::string &nc_path_LUTs, size_t npix)

const get_valid cirrus_mask

#define BT

def center

#define BAD_FLT

const float dBtrefmax

const std::unordered_map< std::string, std::string(*)(const instr *)> get_sst_coeffs_path

flags

void rearrange_stats()

int32_t nbands

size_t operator()(size_t iqual, size_t ilat, size_t idiff, size_t isenz, size_t iquar, size_t iday, size_t isst)

const get_value bt_value

std::vector< float > var_minmax

void get_std_box(const float *inp2d, const int *mask2d, size_t npix, size_t nscan, size_t radius_x, size_t radius_y, float *out, size_t center, l1qstr *l1qrec)

void get_total_2d_max(float *max_global, const float *inp2d, size_t npix, size_t nscan, size_t center, size_t radius)

std::vector< float > bias

float * sst

void copy(double **aout, double **ain, int n)

std::vector< float > bias_out

const float Bt12unif1

const float Bt37unif2

const float Bt40unif1

cldmsk::get_valid get_mask

int ib2

float btrefdiffv6(int32_t ip, float BT39, float BT40, const l1str *l1rec, int fullscanpix)

size_t total_size

const std::unordered_map< std::string, float *(*)(const l1str &)> get_non_BT_vars

const float Bt37unif1

#define BT_LO

void set_maxmin()

l1qstr * l1qrec

#define bool

#define VIIRSJ2

const double scan_time_modis_t_day1

const float Btmax

void set_min()

void get_var_mask(int *mask, const l1str &l1str, size_t npix, int nbands, int ib, get_valid get_mask)

bands

size_t ndiff

std::vector< int > mask_box

const float min_lt

const float Bt40unif2

void radius(double A)

std::vector< float > ratio

int current_scan

#define abs(a)

size_t nsenz

int i

const std::unordered_map< std::string, std::unordered_set< int > > all_sensors

const float dBt4max

void get_var_vals(float *BT, const l1str &l1str, size_t npix, int nbands, int ib, get_value get_val)

const float el_corr_modis_t_2

#define MODISA

#define VIIRSJ1

el

int npix

const float glintmax

cldmsk::get_value get_val

std::vector< float > var_box

const std::unordered_set< int > modis_sensors

std::vector< float > diff

std::unordered_map< std::string, float * > return_vals

void set_max()

l2prod max

const float hisenz

size_t nbands

void rearrange()