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-
- QST DE W1AW
- HR PROPAGATION FORECAST BULLETIN NR 24 ARLP024
- FROM ARRL HEADQUARTERS
- NEWINGTON CT JUN 12, 1989
- TO ALL RADIO AMATEURS
-
- IN THE FIRST TEN DAYS OF JUNE THE SOLAR FLUX GREW FROM 189 TO 266,
- THE LATTER BEING THE HIGHEST SINCE A MARCH 15 PEAK OF 270. THE CYCLE
- 22 HIGH SO FAR IS 299, RECORDED JANUARY 17. A RISING SOLAR FLUX CURVE
- IS NOT NECESSARILY GOOD FOR HF PROPAGATION. INSTEAD, THE DOWN SIDE
- AFTER THE PEAK IS LIKELY TO BRING MORE STABLE CONDITIONS.
-
- THE SPECTACULAR APPEARANCE OF THE SUN ON JUNE 11, AS SEEN THROUGH A
- TELESCOPE EQUIPPED WITH SUITABLE FILTERS FOR VIEWING, INDICATES THAT
- PROPAGATION MAY BE BETTER THIS WEEK THAN SINCE BEFORE THE MARCH FLUX
- PEAK. WHAT MAY BE THE MOST SPECTACULAR SUNSPOT GROUP OF CYCLE 22 TO
- DATE IS POSITIONED FOR MAXIMUM EFFECT THIS WEEK. OTHER SIZABLE GROUPS
- NOW VISIBLE WILL BE AFFECTING PROPAGATION LESS BEFORE THE WEEK IS
- OVER, BUT NOT ENOUGH TO AFFECT THE DX BANDS SERIOUSLY.
-
- PROPAGATION, ESPECIALLY IN THE HIGH LATITUDES OF THE NORTHERN
- HEMISPHERE, HAS BEEN GENERALLY POOR OF LATE. THIS WILL CONTINUE
- THROUGH THE SUMMER, ESPECIALLY ON 21 MHZ AND HIGHER FREQUENCIES. WE
- ARE NEARING THE PEAK TIME FOR SPORADIC E SKIP. THIS MODE MAKES FOR
- STRONG BUT OFTEN ERRATIC SIGNALS OVER RELATIVELY SHORT DISTANCES, THE
- E LAYER BEING NEARER THE EARTH THAN THE F2 LAYER, THE PRIME DX MEDIUM
- IN THE FALL. THE INFLUENCE OF SPORADIC E IS HIGHEST ON 28 AND 50 MHZ,
- BUT IT CAN CAUSE WILD TIMES ON 144 MHZ AS WELL.
-
- E SKIP IS MOST COMMON DURING MID MORNING AND EARLY EVENING HOURS, BUT
- IT CAN APPEAR QUITE SUDDENLY AT ALMOST ANY TIME.
-
- AMERICAN SUNSPOT NUMBERS FOR JUNE 1 THROUGH 7 WERE BETWEEN 117 AND
- 183 WITH A MEAN OF 154R7 AR
-
- QST DE W1AW
- HR PROPAGATION FORECAST BULLETIN NR 24 ARLP024
- FROM ARRL HEADQUARTERS
- NEWINGTON CT JUN 12, 1989
- TO ALL RADIO AMATEURS
-
- IN THE FIRST TEN DAYS OF JUNE THE SOLAR FLUX GREW FROM 189 TO 266,
- THE LATTER BEING THE HIGHEST SINCE A MARCH 15 PEAK OF 270. THE CYCLE
- 22 HIGH SO FAR IS 299, RECORDED JANUARY 17. A RISING SOLAR FLUX CURVE
- IS NOT NECESSARILY GOOD FOR HF PROPAGATION. INSTEAD, THE DOWN SIDE
- AFTER THE PEAK IS LIKELY TO BRING MORE STABLE CONDITIONS.
-
- THE SPECTACULAR APPEARANCE OF THE SUN ON JUNE 11, AS SEEN THROUGH A
- TELESCOPE EQUIPPED WITH SUITABLE FILTERS FOR VIEWING, INDICATES THAT
- PROPAGATION MAY BE BETTER THIS WEEK THAN SINCE BEFORE THE MARCH FLUX
- PEAK. WHAT MAY BE THE MOST SPECTACULAR SUNSPOT GROUP OF CYCLE 22 TO
- DATE IS POSITIONED FOR MAXIMUM EFFECT THIS WEEK. OTHER SIZABLE GROUPS
- NOW VISIBLE WILL BE AFFECTING PROPAGATION LESS BEFORE THE WEEK IS
- OVER, BUT NOT ENOUGH TO AFFECT THE DX BANDS SERIOUSLY.
-
- PROPAGATION, ESPECIALLY IN THE HIGH LATITUDES OF THE NORTHERN
- HEMISPHERE, HAS BEEN GENERALLY POOR OF LATE. THIS WILL CONTINUE
- THROUGH THE SUMMER, ESPECIALLY ON 21 MHZ AND HIGHER FREQUENCIES. WE
- ARE NEARING THE PEAK TIME FOR SPORADIC E SKIP. THIS MODE MAKES FOR
- STRONG BUT OFTEN ERRATIC SIGNALS OVER RELATIVELY SHORT DISTANCES, THE
- E LAYER BEING NEARER THE EARTH THAN THE F2 LAYER, THE PRIME DX MEDIUM
- IN THE FALL. THE INFLUENCE OF SPORADIC E IS HIGHEST ON 28 AND 50 MHZ,
- BUT IT CAN CAUSE WILD TIMES ON 144 MHZ AS WELL.
-
- E SKIP IS MOST COMMON DURING MID MORNING AND EARLY EVENING HOURS, BUT
- IT CAN APPEAR QUITE SUDDENLY AT ALMOST ANY TIME.
-
- AMERICAN SUNSPOT NUMBERS FOR JUNE 1 THROUGH 7 WERE BETWEEN 117 AND
- 183 WITH A MEAN OF 154R7 AR
-