Raffaello Lena,Piergiovanni Salimbeni, Massimo Cicognani, Stefano Basso, A. Bares.

INTRODUCTION
Among the many lunar sites where different visual observers of the past claimed to have recorded a possible LTP, or reflectivity variations, Alphonsus is certainly one of the best known. Tha NSSDC catalog includes all reported phenomena regardless of value of the observation (1-Lunar Transient Phenomena Catalog July 1978 NSSDC W. Cameron  July 1978).
Alphonsus  crater has been reported as the site of Lunar Transient Phenomena (LTP) in the past.

In NSSDC  catalog to the number 705 is reported an event recorded by   Poppendiek, Bond on    1958,  November  19 at    04h 00m - 04h 30m UT.
The observers reported a  diffuse cloud over central mountain, like a plume.
The Physical Data  are reported below

 Date & Time (used in calculations): Nov. 19th 1958 at 04:00 hrs (UT)
 Event position:  Lat. -13.3°  Long. -2.8°
 Event illumination:  Solar Alt.   1.6° over Alphonsus and  Solar Az.   88.7°
 Moon status: Phase 0.60  (Waxing)  Age  8.3d  Colong.   4.6°
 Librations (geocentric):  Lat. -4.7°    Long.  6.5°   Total   8.0°
 The Geologic Lunar Research group (GLR) set out to coordinate its team
of observers for this possible LTP event.

The lighting conditions of that date were to be duplicated
 

Observations

On August 26 a bright spot was recorded by Massimo Cicognani. It appears like a bilobated spot. It appeared to fluctuate sometimes  due to the subtle oscillation of     the seeing.

This observation was carried out under a seeing very poor using a Cassegrain 41 cm f/17.
 

 Massimo Cicognani photo obtained using a Cassegrain 41 cm F/17 . Observation carried out on 26 august 2001 at 20:05 UT
 
 

 This bilobated feature  was observed again by Lena and Salimbeni on October 24 at 21:20 and 20:50 UT respectively
Its albedo estimate was 6.5 on the Elger scale. The peak of Alphonsus  was 8.5 Elger scale. A bilobated  spot very brigth was recorded.

Piergovanni Salimbeni-SCT 20 cm f/10

Raffaello Lena -same date 24 october 2001 at 21:20 UT , Refractor 10 cm f/15 300x.
 

Our conclusion is that the bright effect recorded in 1958 by Poppendick is not  a LTP.

Alphonsus  has some  ridges and hills near the peak along the meridian . These could account for the bright spots bilobated detected by our group.
 
Images carried out for  the GLR project are reported below
  

Stefano Basso, observation carried out on 30 may 2001 at 20:10 UT SCT 20 cm f/10 at 250x.
 

Alessandro Bares  CCD image - mewlon 250 mm.
 

Conclusion:
Small elevations seen under raking sunlight can appear as bright spots .  The whole was an interesting interplay of sunlight and shadow.

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