KF6HI
Contact me through: kf6hi.net


Country Name : Poland (click for all QSOs with this country)

Prefix: SN-SR

Number of QSOs found on 21 MHz with Poland : 21

CallDateTimeModeQSL OUTQSL IN LOTWEQSL
SP1PBW1990-03-2418:34SSBY
Y
NN
SP9PDF1990-03-2418:48SSBY
Y
NN
SO3IF1992-10-2414:33SSBNNNN
3Z25PAZ1992-10-2416:45SSBYNNN
SP9LJD1992-10-2518:11SSBY
Y
NN
SP7ZET1993-03-0715:23SSBNNNN
SN3A1993-03-0716:36SSBNNNN
SP9LJD1993-03-0717:19SSBNNNN
SP6YAQ1993-03-0717:41SSBNNNN
SO2R2012-10-2816:19SSBNNNN
SP8PFK2012-10-2817:09SSBNNNN
SO2R2012-10-2817:55SSBNNNN
SO9Q2012-10-2818:16SSBNN
V
N
SP3S2012-10-2818:20SSBNN
Y
N
SN2M2014-02-1515:39CWNN
Y
N
SP8R2014-02-1515:41CWNNNN
SN5X2014-02-1515:42CWNN
Y
N
SP9LJN2016-02-2115:44CWNNNN
SN7Q2016-09-2416:23RTTYNN
Y
N
SN7Q2023-02-1817:32CWNN
Y
N
3Z1K2023-02-1818:19CWNNNN

KF6HI QSO with SN3A (click for QRZ info), information for above highlighted contact:

UTC Date: 1993-Mar-07
UTC Time: 16:36
Frequency: 21.000 MHz
Report Sent: 59
Report Received: 59
Mode: SSB
Sunspot Number (>0): 93
Solar Flux (>67): 150
A-index (0-400): 27
3-hour K-index (0-9): 4.44
KF6HI
Sunrise 14:15
Sunset 01:56

SN3A
Sunrise 05:14
Sunset 16:32
Grid:
ADIF code: 269
WAZ Zone: 15
Continent: EU
Latitude: 51.77 °
Longitude: -19.50 °
Bearing 24 °
Distance(km): 9623
Distance(miles): 5975
Operator:
Comments:
QSL info:
Record Number: 5513

LP=Long Path if shown
Map Legend: =Home, =DX Station, =Sun Position
Red line = Communications path


The day/night terminator has 4 shade levels going from light to dark
  • Twilight or dusk is where the sun is 6° below the horizon. The D layer (green line at right) is illumiated is this area and to 9° below the horizon.
  • Nautical twilight the sun is 12° below the horizon; the horizon is still visible,
  • Astronomical twilight sun is 18° below the horizon The F layer (red line at right) is illumiated is this area and to 20° below the horizon.
  • Night
The Magnetic Equator is shown as a black line around the 0 degree equator line
The Magnetic Equator is important for Transequatorial Propogation and the magnetic field strengths are believed to be important for Sporadic-E Propagation.
Verifications: