mirror of
https://github.com/f4exb/sdrangel.git
synced 2024-11-27 02:09:14 -05:00
253 lines
8.6 KiB
C++
253 lines
8.6 KiB
C++
///////////////////////////////////////////////////////////////////////////////////
|
|
// Copyright (C) 2017 Edouard Griffiths, F4EXB. //
|
|
// Copyright (C) 2021 Jon Beniston, M7RCE //
|
|
// //
|
|
// This program is free software; you can redistribute it and/or modify //
|
|
// it under the terms of the GNU General Public License as published by //
|
|
// the Free Software Foundation as version 3 of the License, or //
|
|
// (at your option) any later version. //
|
|
// //
|
|
// This program is distributed in the hope that it will be useful, //
|
|
// but WITHOUT ANY WARRANTY; without even the implied warranty of //
|
|
// MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the //
|
|
// GNU General Public License V3 for more details. //
|
|
// //
|
|
// You should have received a copy of the GNU General Public License //
|
|
// along with this program. If not, see <http://www.gnu.org/licenses/>. //
|
|
///////////////////////////////////////////////////////////////////////////////////
|
|
|
|
#ifndef INCLUDE_RADIOASTRONOMYSETTINGS_H
|
|
#define INCLUDE_RADIOASTRONOMYSETTINGS_H
|
|
|
|
#include <QByteArray>
|
|
#include <QString>
|
|
#include <QDateTime>
|
|
|
|
#include "dsp/dsptypes.h"
|
|
|
|
class Serializable;
|
|
|
|
// Number of columns in the tables
|
|
#define RADIOASTRONOMY_POWERTABLE_COLUMNS 28
|
|
|
|
// Number of sensors
|
|
#define RADIOASTRONOMY_SENSORS 2
|
|
|
|
struct RadioAstronomySettings
|
|
{
|
|
struct AvailableFeature
|
|
{
|
|
int m_featureSetIndex;
|
|
int m_featureIndex;
|
|
QString m_type;
|
|
|
|
AvailableFeature() = default;
|
|
AvailableFeature(const AvailableFeature&) = default;
|
|
AvailableFeature& operator=(const AvailableFeature&) = default;
|
|
bool operator==(const AvailableFeature& a) const {
|
|
return (m_featureSetIndex == a.m_featureSetIndex) && (m_featureIndex == a.m_featureIndex) && (m_type == a.m_type);
|
|
}
|
|
};
|
|
|
|
int m_inputFrequencyOffset;
|
|
int m_sampleRate;
|
|
int m_rfBandwidth;
|
|
int m_integration; //!< Number of samples to integrate
|
|
|
|
int m_fftSize;
|
|
enum FFTWindow {
|
|
REC,
|
|
HAN
|
|
} m_fftWindow; //!< FFT windowing function
|
|
QString m_filterFreqs; //!< List of channels (bin indices) to filter in FFT to remove RFI
|
|
|
|
QString m_starTracker; //!< Name of Star Tracker plugin to link with
|
|
QString m_rotator; //!< Name of antenna rotator
|
|
|
|
float m_tempRX; //!< Receiver noise temperature in K (Front end NF)
|
|
float m_tempCMB; //!< Cosmic microwave background temperature in K
|
|
float m_tempGal; //!< Galactic background temperature in K
|
|
float m_tempSP; //!< Spillover temperature in K
|
|
float m_tempAtm; //!< Atmospheric temperature in K
|
|
float m_tempAir; //!< Surface air temperature in C
|
|
float m_zenithOpacity; //!< Opacity of atmosphere at zenith
|
|
float m_elevation; //!< Elevation in degrees, if not using value from Star Tracker
|
|
bool m_tempGalLink;
|
|
bool m_tempAtmLink;
|
|
bool m_tempAirLink;
|
|
bool m_elevationLink;
|
|
|
|
float m_gainVariation; //!< delta G/G
|
|
enum SourceType {
|
|
UNKNOWN,
|
|
COMPACT,
|
|
EXTENDED,
|
|
SUN,
|
|
CAS_A
|
|
} m_sourceType; //!< Whether the source it smaller than the beam
|
|
float m_omegaS; //!< Source angle
|
|
enum AngleUnits {
|
|
DEGREES,
|
|
STERRADIANS
|
|
} m_omegaSUnits;
|
|
enum AngleUnits m_omegaAUnits;
|
|
|
|
bool m_spectrumPeaks;
|
|
bool m_spectrumMarkers;
|
|
bool m_spectrumTemp;
|
|
bool m_spectrumReverseXAxis;
|
|
bool m_spectrumRefLine;
|
|
bool m_spectrumLAB;
|
|
bool m_spectrumDistance;
|
|
bool m_spectrumLegend;
|
|
float m_spectrumReference; //!< In dB
|
|
float m_spectrumRange; //!< In dB
|
|
float m_spectrumSpan; //!< In Mhz
|
|
float m_spectrumCenterFreqOffset; //!< Offset - rather than absolute - In Mhz
|
|
bool m_spectrumAutoscale;
|
|
enum SpectrumYScale {
|
|
SY_DBFS,
|
|
SY_SNR,
|
|
SY_DBM,
|
|
SY_TSYS,
|
|
SY_TSOURCE
|
|
} m_spectrumYScale;
|
|
enum SpectrumBaseline {
|
|
SBL_TSYS0,
|
|
SBL_TMIN,
|
|
SBL_CAL_COLD
|
|
} m_spectrumBaseline;
|
|
bool m_recalibrate;
|
|
float m_tCalHot; //!< Hot calibration antenna noise temperature in K (Sky + Spillover?)
|
|
float m_tCalCold; //!< Cold calibration antenna noise temperature in K
|
|
enum Line {
|
|
HI,
|
|
OH,
|
|
DI,
|
|
CUSTOM_LINE
|
|
} m_line; //!< Spectral line to plot and use as Doppler reference
|
|
float m_lineCustomFrequency; //!< Spectral line frequency when m_line==CUSTOM
|
|
enum RefFrame {
|
|
TOPOCENTRIC,
|
|
BCRS,
|
|
LSR
|
|
} m_refFrame; //!< Reference frame for velocities
|
|
|
|
float m_sunDistanceToGC; //!< Sun distance to Galactic Center In kpc
|
|
float m_sunOrbitalVelocity; //!< In km/s around GC
|
|
|
|
bool m_powerPeaks;
|
|
bool m_powerMarkers;
|
|
bool m_powerAvg;
|
|
bool m_powerLegend;
|
|
bool m_powerShowTsys0; //!< Plot total noise temperature
|
|
bool m_powerShowAirTemp;
|
|
bool m_powerShowGaussian;
|
|
bool m_powerShowFiltered;
|
|
bool m_powerShowMeasurement;
|
|
float m_powerReference; //!< In dB
|
|
float m_powerRange; //!< In dB
|
|
bool m_powerAutoscale;
|
|
enum PowerYData {
|
|
PY_POWER,
|
|
PY_TSYS,
|
|
PY_TSOURCE,
|
|
PY_FLUX,
|
|
PY_2D_MAP
|
|
} m_powerYData;
|
|
enum PowerYUnits {
|
|
PY_DBFS,
|
|
PY_DBM,
|
|
PY_WATTS,
|
|
PY_KELVIN,
|
|
PY_SFU,
|
|
PY_JANSKY
|
|
} m_powerYUnits;
|
|
enum PowerFilter {
|
|
FILT_MEDIAN,
|
|
FILT_MOVING_AVERAGE,
|
|
// TODO: FILT_LPF
|
|
} m_powerFilter;
|
|
int m_powerFilterN;
|
|
|
|
enum SweepType {
|
|
SWP_AZEL,
|
|
SWP_LB,
|
|
SWP_OFFSET
|
|
};
|
|
|
|
bool m_power2DLinkSweep; //<! Update setting below to match sweep parameters
|
|
SweepType m_power2DSweepType;
|
|
int m_power2DWidth;
|
|
int m_power2DHeight;
|
|
float m_power2DXMin;
|
|
float m_power2DXMax;
|
|
float m_power2DYMin;
|
|
float m_power2DYMax;
|
|
bool m_powerColourAutoscale;
|
|
float m_powerColourScaleMin;
|
|
float m_powerColourScaleMax;
|
|
QString m_powerColourPalette;
|
|
|
|
enum RunMode {
|
|
SINGLE,
|
|
CONTINUOUS,
|
|
SWEEP
|
|
} m_runMode;
|
|
bool m_sweepStartAtTime;
|
|
QDateTime m_sweepStartDateTime;
|
|
SweepType m_sweepType;
|
|
float m_sweep1Start;
|
|
float m_sweep1Stop;
|
|
float m_sweep1Step;
|
|
float m_sweep1Delay; //!< Delay after rotation before a measurement
|
|
float m_sweep2Start;
|
|
float m_sweep2Stop;
|
|
float m_sweep2Step;
|
|
float m_sweep2Delay; //!< Delay after a measurement before starting the next
|
|
|
|
QString m_sensorName[RADIOASTRONOMY_SENSORS];
|
|
QString m_sensorDevice[RADIOASTRONOMY_SENSORS];
|
|
QString m_sensorInit[RADIOASTRONOMY_SENSORS];
|
|
QString m_sensorMeasure[RADIOASTRONOMY_SENSORS];
|
|
bool m_sensorEnabled[RADIOASTRONOMY_SENSORS];
|
|
bool m_sensorVisible[RADIOASTRONOMY_SENSORS];
|
|
float m_sensorMeasurePeriod;
|
|
|
|
bool m_gpioEnabled;
|
|
int m_gpioPin;
|
|
int m_gpioSense;
|
|
QString m_startCalCommand;
|
|
QString m_stopCalCommand;
|
|
float m_calCommandDelay; //!< Delay in seconds after command before starting cal
|
|
|
|
quint32 m_rgbColor;
|
|
QString m_title;
|
|
Serializable *m_channelMarker;
|
|
Serializable *m_rollupState;
|
|
int m_streamIndex; //!< MIMO channel. Not relevant when connected to SI (single Rx).
|
|
bool m_useReverseAPI;
|
|
QString m_reverseAPIAddress;
|
|
uint16_t m_reverseAPIPort;
|
|
uint16_t m_reverseAPIDeviceIndex;
|
|
uint16_t m_reverseAPIChannelIndex;
|
|
int m_workspaceIndex;
|
|
QByteArray m_geometryBytes;
|
|
bool m_hidden;
|
|
|
|
int m_powerTableColumnIndexes[RADIOASTRONOMY_POWERTABLE_COLUMNS];//!< How the columns are ordered in the table
|
|
int m_powerTableColumnSizes[RADIOASTRONOMY_POWERTABLE_COLUMNS]; //!< Size of the columns in the table
|
|
|
|
RadioAstronomySettings();
|
|
void resetToDefaults();
|
|
void setChannelMarker(Serializable *channelMarker) { m_channelMarker = channelMarker; }
|
|
void setRollupState(Serializable *rollupState) { m_rollupState = rollupState; }
|
|
QByteArray serialize() const;
|
|
bool deserialize(const QByteArray& data);
|
|
|
|
static const QStringList m_pipeTypes;
|
|
static const QStringList m_pipeURIs;
|
|
};
|
|
|
|
#endif /* INCLUDE_RADIOASTRONOMYSETTINGS_H */
|