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			97 lines
		
	
	
		
			3.4 KiB
		
	
	
	
		
			C++
		
	
	
	
	
	
			
		
		
	
	
			97 lines
		
	
	
		
			3.4 KiB
		
	
	
	
		
			C++
		
	
	
	
	
	
| ///////////////////////////////////////////////////////////////////////////////////
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| // Copyright (C) 2023 Jon Beniston, M7RCE                                        //
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| //                                                                               //
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| // This program is free software; you can redistribute it and/or modify          //
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| // it under the terms of the GNU General Public License as published by          //
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| // the Free Software Foundation as version 3 of the License, or                  //
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| // (at your option) any later version.                                           //
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| //                                                                               //
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| // This program is distributed in the hope that it will be useful,               //
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| // but WITHOUT ANY WARRANTY; without even the implied warranty of                //
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| // MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the                  //
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| // GNU General Public License V3 for more details.                               //
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| //                                                                               //
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| // You should have received a copy of the GNU General Public License             //
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| // along with this program. If not, see <http://www.gnu.org/licenses/>.          //
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| ///////////////////////////////////////////////////////////////////////////////////
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| 
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| #ifndef INCLUDE_GOESXRAY_H
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| #define INCLUDE_GOESXRAY_H
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| 
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| #include <QtCore>
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| #include <QTimer>
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| #include <QJsonObject>
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| 
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| #include "export.h"
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| 
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| class QNetworkAccessManager;
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| class QNetworkReply;
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| 
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| // GOES X-Ray data
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| // This gets 1-minute averages of solar X-rays the 1-8 Angstrom (0.1-0.8 nm) and 0.5-4.0 Angstrom (0.05-0.4 nm) passbands from the GOES satellites
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| // https://www.swpc.noaa.gov/products/goes-x-ray-flux
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| // There are primary and secondary data sources, from different satellites, as sometimes they can be in eclipse
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| // Also gets Proton flux (Which may be observed on Earth a couple of days after a large flare/CME)
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| class SDRBASE_API GOESXRay : public QObject
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| {
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|     Q_OBJECT
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| protected:
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|     GOESXRay();
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| 
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| public:
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|     struct XRayData {
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|         QDateTime m_dateTime;
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|         QString m_satellite;
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|         double m_flux;
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|         enum Band {
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|             UNKNOWN,
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|             SHORT,  // 0.05-0.4nm
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|             LONG    // 0.1-0.8nm
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|         } m_band;
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|         XRayData() :
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|             m_flux(NAN),
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|             m_band(UNKNOWN)
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|         {
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|         }
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|     };
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| 
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|     struct ProtonData {
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|         QDateTime m_dateTime;
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|         QString m_satellite;
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|         double m_flux;
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|         int m_energy; // 10=10MeV, 50MeV, 100MeV, 500MeV
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|         ProtonData() :
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|             m_flux(NAN),
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|             m_energy(0)
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|         {
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|         }
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|     };
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| 
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|     static GOESXRay* create(const QString& service="services.swpc.noaa.gov");
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| 
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|     ~GOESXRay();
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|     void getDataPeriodically(int periodInMins=10);
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| 
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| public slots:
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|     void getData();
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| 
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| private slots:
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|     void handleReply(QNetworkReply* reply);
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| 
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| signals:
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|     void xRayDataUpdated(const QList<GOESXRay::XRayData>& data, bool primary);  // Called when new data available.
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|     void protonDataUpdated(const QList<GOESXRay::ProtonData> &data, bool primary);
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| 
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| private:
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|     bool containsNonNull(const QJsonObject& obj, const QString &key) const;
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|     void handleXRayJson(const QByteArray& bytes, bool primary);
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|     void handleProtonJson(const QByteArray& bytes, bool primary);
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| 
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|     QTimer m_dataTimer;             // Timer for periodic updates
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|     QNetworkAccessManager *m_networkManager;
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| 
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| };
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| 
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| #endif /* INCLUDE_GOESXRAY_H */
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| 
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