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The original message has been attached to this so you can view it (if it isn't spam) or label similar future email. If you have any questions, see the administrator of that system for details. Content preview: Here is some further info for discussion on WSPR vs. OP. On 8/23/12 WD2XES and WD2XNS conducted a 'heads up' test of WSPR vs OP4 on 136 kHz. The test started at 2230Z on 8/23/12 (in daylight), continued throughout the night, and concluded at 1030Z on 8/24/12 (in daylight). Conditions were normal for a summer evening with typical amounts of static. Distance between XES and XNS is 72 miles. [...] Content analysis details: (4.4 points, 5.0 required) pts rule name description ---- ---------------------- -------------------------------------------------- -0.0 RCVD_IN_DNSWL_NONE RBL: Sender listed at http://www.dnswl.org/, no trust [76.96.62.48 listed in list.dnswl.org] 0.2 STOX_REPLY_TYPE STOX_REPLY_TYPE 0.0 FREEMAIL_FROM Sender email is commonly abused enduser mail provider (jrusgrove[at]comcast.net) -0.0 SPF_PASS SPF: sender matches SPF record -0.7 RP_MATCHES_RCVD Envelope sender domain matches handover relay domain 1.9 STOX_REPLY_TYPE_WITHOUT_QUOTES STOX_REPLY_TYPE_WITHOUT_QUOTES 3.1 AXB_XMAILER_MIMEOLE_OL_4379D AXB_XMAILER_MIMEOLE_OL_4379D X-Scan-Signature: a6b6ffaf48fdddf1ed5c25dc4bf03ee1 Subject: LF: WSPR vs. Opera Content-Type: text/plain; format=flowed; charset="iso-8859-1"; reply-type=original Content-Transfer-Encoding: 7bit X-Spam-Checker-Version: SpamAssassin 2.63 (2004-01-11) on post.thorcom.com X-Spam-Level: X-Spam-Status: No, hits=0.3 required=5.0 tests=NO_REAL_NAME autolearn=no version=2.63 X-SA-Exim-Scanned: Yes Sender: owner-rsgb_lf_group@blacksheep.org Precedence: bulk Reply-To: rsgb_lf_group@blacksheep.org X-Listname: rsgb_lf_group X-SA-Exim-Rcpt-To: rs_out_1@blacksheep.org X-SA-Exim-Scanned: No; SAEximRunCond expanded to false x-aol-global-disposition: G x-aol-sid: 3039ac1d61855088a0be1d89 X-AOL-IP: 195.171.43.25 X-AOL-SPF: domain : blacksheep.org SPF : none Here is some further info for discussion on WSPR vs. OP. On 8/23/12 WD2XES and WD2XNS conducted a 'heads up' test of WSPR vs OP4 on 136 kHz. The test started at 2230Z on 8/23/12 (in daylight), continued throughout the night, and concluded at 1030Z on 8/24/12 (in daylight). Conditions were normal for a summer evening with typical amounts of static. Distance between XES and XNS is 72 miles. At the WD2XES transmitting end John combined both WSPR and OP4 signals into a common phasing transmitter, amplifier and transmitting antenna. Transmitted power levels were identical for each mode and very QRP - 60 mW or less. WSPR and OP4 frequencies were within a kHz of each other. At the WD2XNS receiving end a common receiving antenna was used feeding a single GPS disciplined receiver. Audio output from the receiver was applied to a single sound card / computer setup which ran an instance of each program. Results can be found at http://www.w1vd.com/WSPROP4082312A.pdf . Notes: 1) At 0230Z John made a significant reduction in transmitted power level to better explore the weak signal performance of the two modes. This produced the desired results with 'at the threshold' receptions through 0420Z. No receptions were noted between 0420Z to 0902Z and were probably due to an increased static level during that period. Signals climbed back out of the noise again at 0902Z and reception continued through the testing period. 2) The OP4 results were 'time shifted' to align with the corresponding WSPR start times. 3) There are a few instances where the OP4 results are not spaced on exactly 4 minute intervals ... this is likely caused by Opera reporting 'slipping' into the following minute. Conclusion: WSPR has an advantage over OP4 in weak signal performance. Also, keep in mind that WSPR requires half the amount of transmission time and transmits more information. In our opinion, OP8 would be more in line with WSPR in terms of weak signal performance. In that case WSPR gets the job done in one fourth the time taken by OP8 and transmits more information. Jay W1VD WD2XNS WE2XGR/2 John W1TAG WD2XES WE2XGR/3