We report several observations of the Lα interplanetary emission recorded by a photometer flown in 1977 on board the soviet spacecraft Prognoz‐5. The Prognoz scans sampled emission in a plane perpendicular to the sun‐spacecraft line and also traversed the Lα maximum emission region (MER), a region centered a few AU from the Sun on the upstream interstellar‐flow axis. These scans reveal the existence of a 10% decrease in intensity centered near the ecliptic plane and about 30° wide. All the dips form a new feature of the interplanetary emission, a “groove” aligned approximately with the ecliptic plane. This groove is present only near the upwind direction, and is interpreted as the result of enhanced ionisation of interstellar H by charge‐exchange with the solar wind in a sheet of approximately 30° width in latitude around the average position of the neutral sheet, at this time of solar minimum.